The galaxy appears to be in a complex system, possibly an interacting group. The brightest component exhibits a largely smooth morphology, with a generally elliptical shape. There is evidence of an extended halo surrounding this central body.

Another component presents a disk-like structure with hints of spiral arms, displaying a bluer color, suggestive of ongoing star formation.

A third, fainter component shows a more irregular morphology, possibly indicating tidal disruption or recent interaction. There are signs of tidal bridges or streams connecting these components, further supporting the hypothesis of an interacting system. The overall color profile suggests a mix of older stellar populations in the smooth component and younger, bluer stars in the disk component.
