The galaxy exhibits a morphology that suggests an ongoing or recent merger event. The primary body of the galaxy appears relatively smooth and somewhat rounded, with a diffuse halo of light extending outwards. There is evidence of a secondary, brighter core within the galaxy, potentially indicative of the nucleus of the merging companion. The overall color profile suggests a mixed stellar population. The presence of bluer hues in certain regions could be indicative of ongoing star formation, potentially triggered by the interaction. Patches of yellow and redder light are apparent, suggesting the presence of older stellar populations or dust obscuration within the system. The overall structure displays some degree of asymmetry, further supporting the hypothesis of a recent or ongoing interaction. There appears to be tidal tails or other disrupted features, although these are faint and not clearly defined.
