The galaxy presents as a system undergoing a significant interaction, possibly a merger. The primary body displays a relatively smooth, elliptical morphology with a concentrated central bulge. There is evidence of a tidal tail or plume extending from the main body, suggesting gravitational disturbance. The color gradient indicates older stellar populations within the main body, trending toward bluer regions in the disturbed areas, potentially indicative of ongoing or recent star formation triggered by the interaction. The overall light distribution reveals a complex structure, not a simple elliptical or spiral form, implying a dynamic state.
