The galaxy appears as a centrally concentrated system with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-white hue, suggesting an older stellar population. The light gradually fades into a dimmer, reddish halo extending outwards from the center. This extended halo lacks any discernible spiral arm structure or dust lanes, and it is characterized by a fairly uniform distribution of light. The overall appearance is largely undisturbed, showing no signs of major tidal interactions or significant mergers. Slight asymmetry is noted in the light distribution of the outer regions.