The galaxy presents a generally smooth, elliptical morphology. The light profile suggests a highly concentrated nucleus, with a gradual decrease in luminosity outward. The central region exhibits a yellowish-white color, potentially indicating an older stellar population. No distinct spiral arms or prominent dust lanes are visible. The outer regions fade gradually into the background, exhibiting a faint bluish-white hue, possibly indicative of some low-level star formation activity in the extended halo. There is no obvious sign of tidal disturbances or recent merger activity. The galaxy appears as a relatively undisturbed system.
