The galaxy presents an ambiguous morphology, potentially indicative of a disturbed system. The primary body of the galaxy exhibits a somewhat elliptical profile, with a relatively smooth texture. There is a notable extension or plume emanating from the main body, suggesting a possible tidal feature. The color gradient appears consistent with an older stellar population, with a generally redder hue throughout. However, there are localized areas of slightly bluer color in the plume. The structure seems to be undergoing a merger, likely a later stage merger.
