The galaxy presents as a merging system, exhibiting significant tidal features and disturbed morphology. The primary galaxy appears relatively smooth and elliptical in shape, with a concentrated central bulge. A secondary, smaller component is situated nearby, displaying a more irregular shape and a yellowish hue, suggestive of an older stellar population. The interaction between the two galaxies is evident in the diffuse, extended halo surrounding the system, potentially indicative of tidal stripping and gravitational disruption. There are several distinct clumps that likely signify ongoing regions of star formation within this merger. Overall, this galaxy appears to be undergoing a significant transformation as a result of an ongoing or recent merger event.
