The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. The overall light distribution is disturbed, with two distinct, bright central concentrations that likely correspond to the cores of the merging galaxies. These cores are slightly elliptical in shape and exhibit a yellowish-orange hue, potentially indicative of an older stellar population. Diffuse tidal features are visible extending outwards from the main body of the galaxy, with a faint bluish tint, indicative of some star formation occurring in these extended regions. The overall structure appears to be relatively compact.
