The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. A prominent bulge dominates the central region, displaying a yellowish-orange hue, potentially indicative of an older stellar population. The galaxy lacks any readily apparent spiral arm structure or significant dust lanes. There is a subtle extension of the galactic light outwards from the central bulge, forming a diffuse halo. Overall, the galaxy appears relatively undisturbed, lacking signs of recent major merger activity or tidal distortions. The observed color and morphology suggest that the galaxy is undergoing relatively low levels of star formation.