The galaxy exhibits a disk-like morphology, though with significant irregularities in its structure. While not a classic spiral, there are hints of spiral arm structures, but these are ill-defined and appear more flocculent. The galaxy presents an overall patchy appearance, with several distinct knots of bluer light, suggestive of active star formation regions. The color index is shifted towards the blue end of the spectrum, indicative of a younger stellar population. The central bulge is either very small or nearly non-existent, with the majority of the galaxy's light emanating from the disk. The overall distribution of light suggests this galaxy may be undergoing some form of interaction or disturbance, disrupting its regular structure. There appears to be a faint, diffuse halo surrounding the central region. No strong bar feature is clearly visible. The galaxy’s disk is oriented at an oblique angle relative to our line of sight. There is a possibility that the galaxy is undergoing minor to major merging with a companion galaxy.
