The galaxy presents a complex, multi-component structure suggestive of an ongoing or recent interaction/merger event. The primary body of the galaxy appears relatively smooth, with a somewhat rounded morphology, although not perfectly spherical. There are indications of disturbed features, possibly tidal tails or debris, extending from the main body. The color gradient suggests a mixed stellar population, with a dominant older population. The galaxy exhibits moderate star formation activity. The observed features may indicate that this system is in a late stage of merging.
