The galaxy presents a predominantly smooth morphology. The central bulge exhibits a bright, concentrated luminosity, appearing yellowish-white in color. Moving outward from the bulge, a fainter disk is discernible, oriented at a slight angle to our line of sight. The disk appears mottled, with subtle variations in surface brightness, hinting at possible underlying spiral arm structure, though not sharply defined. The overall color of the disk is slightly bluer than the central bulge, suggestive of younger stellar populations. There are no obvious signs of major mergers or tidal disturbances, but there are hints of minor disturbance that indicate a merger. The galaxy's profile gradually fades into the background sky, implying a relatively undisturbed and evolved system.
