The galaxy presents as a somewhat smooth, though notably disturbed, structure. Its overall shape tends toward round, but also exhibits intermediate characteristics, suggesting a departure from a perfect elliptical form. The light distribution is concentrated, with a brighter, more intense core, fading outward toward less defined edges. The color profile exhibits a reddish-orange hue, which may indicate an older stellar population or significant dust obscuration. There are possible indications of minor tidal disturbances or interactions within the system, though these are not pronounced. There is a possible merging event occurring. These merging signatures take the form of asymmetries in the light distribution. The galaxy does not show a definitive disk structure, but has a slight amount of blue light being emitted.
