The galaxy presents as a diffuse, elliptical object. The central region exhibits a bright, concentrated luminosity, suggesting a substantial stellar density, most likely consistent with an older stellar population. The light falls off smoothly from the core. The outer regions of the galaxy are less defined, fading into the background sky. There is a slight indication of a disk-like structure around the core, but the overall morphology is dominated by its elliptical shape and smooth appearance, with no spiral arms or dust lanes discernible. The galaxy's color profile appears relatively uniform, with a slightly bluer hue that may indicate some ongoing star formation. There is no evidence of any recent or ongoing major mergers, although there is an indication of some minor disturbances in the outer disc of the galaxy.
