The galaxy exhibits a relatively smooth, elliptical morphology with a slight central bulge. There is evidence of a disk-like structure, although it appears less prominent and somewhat disturbed, hinting at possible interactions. The color profile suggests a stellar population that is primarily evolved, with the central region displaying a yellowish-orange hue, indicating older stars. There might be some regions of recent or ongoing star formation present along the edges of the disk, marked by a slightly bluer color, though these areas are not very pronounced. The overall structure of the galaxy does not indicate a major ongoing merger, but there are subtle signs of possible minor disturbances in the disk, which could be remnants of a past interaction or a potential minor merger event.
