The galaxy presents a roughly elliptical morphology, although exhibiting signs of disturbance. The light distribution suggests a concentrated core, with a radial profile that diminishes smoothly outwards. The galaxy displays a redder hue toward the center and shows slightly bluer regions extending towards the outer edges, implying possible differences in stellar population and age. The central bulge appears significant, lending further weight to the early-type galaxy characterization, albeit with potential ongoing star formation or recent interactions influencing the bluer outskirts. A slight asymmetry is noticeable in the overall shape, which may be indicative of tidal interactions or a minor merger event.
