The galaxy presents as a system comprised of distinct concentrations of luminosity. The primary morphology appears to be elliptical, although evidence suggests the potential presence of an ongoing or recent merger. At least three such distinct luminous areas can be identified. The individual structures are roughly circular, exhibiting a gradient of brightness decreasing outward from the center. Overall, the galaxy exhibits a generally smooth appearance. Coloration appears to be dominated by yellow and red, suggesting a population of older stars. There may be ongoing star formation, but it is likely at a low rate. The mass estimates and colours indicate this is a relatively massive galaxy that is fairly red, meaning it's populated by relatively old stars. The disturbance also suggests ongoing interactions.
