The galaxy presents as a smooth, elliptical-like structure with a notable central bulge. The color profile suggests an aging stellar population, with a yellowish-orange hue dominating the core, indicative of older, redder stars. There is a slight color gradient moving outward from the core, with a faint bluish-white tinge suggesting the presence of some younger stars or possibly a low level of ongoing star formation in the outer regions. No spiral arms or distinct dust lanes are readily apparent. The galaxy's light is generally evenly distributed, with a gradual decline in surface brightness from the center towards the edges, consistent with an early-type galaxy.
