The galaxy presents as a resolved object, with a complex morphology suggestive of possible interaction. The main body exhibits a relatively smooth central region, but with discernible features indicating a more complex structure than a purely elliptical galaxy. There is an indication of disk-like morphology. The color distribution shows a trend with bluer colors concentrated towards the galaxy's central parts, transitioning towards redder colors as it extends outward, which may point to younger stellar populations dominating the core and older ones in the outer regions. The overall shape is neither strictly spherical nor elliptical, but rather presents a more irregular form. There are some signs of minor distortions, but no strong indication of a large ongoing merger event.
