The galaxy presents as a fairly compact, elliptical or spheroidal galaxy, exhibiting a smooth, centrally concentrated luminosity profile. The core region demonstrates a bright yellowish-white hue, indicative of an older stellar population. The overall structure is relatively featureless, lacking prominent spiral arms or distinct dust lanes. There is a subtle color gradient as you move outwards from the center, with the outer regions appearing slightly redder, suggesting a possible gradient in stellar age or metallicity. The galaxy appears to be relatively undisturbed with no signs of major mergers or tidal interactions. Its round morphology suggests a relaxed system, possibly resulting from a long period of isolated evolution. The low level of star formation indicated by the overall color further supports this classification as an evolved system.