The galaxy presents a relatively smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity suggesting a high density of stars or an active galactic nucleus. There is a noticeable redder color in the central region, potentially indicating an older stellar population. The overall color profile shifts towards bluer hues in the outer regions, hinting at ongoing star formation or a younger stellar population in the galactic disk. The galaxy appears to be undergoing a merger event, with a possible tidal tail or disturbed morphology indicating gravitational interactions.
