The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile. The core region is dominated by a bright, yellowish-white hue, indicative of an older stellar population. Extending outwards from the core, a fainter, bluer halo is visible. This halo suggests the presence of some younger stars and possibly ongoing, though limited, star formation within the galaxy. The overall structure appears undisturbed, showing no signs of major mergers or tidal interactions. The galaxy's shape is slightly elongated, but not excessively so, suggesting a moderate degree of ellipticity. Faint color variations are present within the halo, implying some heterogeneity in stellar populations or dust content.
