This galaxy presents a complex morphology, appearing as a system potentially undergoing a merging event or exhibiting significant tidal interactions. The primary component of the galaxy displays a somewhat irregular, disturbed structure, with noticeable asymmetries in its light distribution. A diffuse, extended halo surrounds the main body, suggesting possible disruption from gravitational interactions.

There are visible features indicative of on-going star formation, namely patches of bluer light distributed across the central and outer regions, which may signify areas of active star birth. These regions appear superimposed on an underlying, older stellar population, indicated by more reddish hues throughout the galaxy. The overall color of the galaxy leans toward the redder end of the spectrum, suggesting a significant population of evolved stars, though the blue knots indicate the presence of younger stellar populations as well.

The galaxy's shape is neither fully elliptical nor spiral; rather it exhibits an irregular form. There is a central concentration of light that could represent a galactic bulge, though it lacks the smooth appearance associated with classic elliptical galaxies. Faint, extended structures emerge from the main galactic body which could be tidal tails or disrupted spiral arms. The presence of these features, in conjunction with the disturbed morphology, suggests that this system is not dynamically relaxed.
