The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density. The overall color appears slightly redder, indicative of a population dominated by older, cooler stars. There may be a slight asymmetry to the galaxy's shape, although this is difficult to ascertain definitively from the image resolution, potentially from a minor disturbance. There is no clear evidence of a prominent disk, spiral arms, or significant dust lanes. The galaxy appears relatively undisturbed with perhaps some minor disturbances, suggesting it may be in a more evolved stage of its lifecycle.
