This galaxy exhibits a complex morphology. The overall form suggests a merging system, or a galaxy undergoing significant tidal disruption. A bright, roughly circular component dominates the western side. It shows a yellow hue. To the east, a distorted structure extends outward, displaying a more reddish color, perhaps indicative of older stellar populations or significant dust obscuration. This structure appears elongated, with evidence of tidal tails or streams extending away from the central region. There is a hint of a less-defined secondary nucleus or dense region embedded within this eastern structure. The light distribution within the galaxy is not uniform. It may have smooth features along with indications of disk-like attributes. There is the possibility of ongoing or past interactions that have disturbed the galaxy's original structure.
