The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth, diffuse halo. Its core exhibits a bright, yellowish hue that gradually fades into the surrounding, less luminous regions. The observed color suggests a stellar population dominated by older, redder stars. There is a slight elongation along one axis, hinting at a possible deviation from a perfectly spherical shape, but it is largely rounded. No distinct spiral arms or significant dust lanes are visible. Minimal disturbances or tidal features are observed, suggesting that this is a relaxed galaxy without significant mergers. 
