The galaxy appears to be a single, relatively smooth object with a concentrated central region. It exhibits a generally elliptical morphology, with an aspect ratio that suggests it is nearly circular in projection. The color profile is slightly redder in the central regions, transitioning to a bluer hue towards the outer edges, indicating possible variations in stellar populations. There is no visually apparent spiral structure or evidence of ongoing major merger activity, although faint tidal features or minor disturbances cannot be entirely ruled out given the image resolution. Overall, the galaxy is consistent with a massive early-type galaxy undergoing a low level of star formation.
