The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a predominantly yellowish hue, suggesting an older stellar population with minimal ongoing star formation. There are no apparent spiral arm structures or prominent dust lanes visible in this observation. The galaxy appears generally round in shape, with no significant morphological distortions indicative of recent major merger events. Faint extensions of light surround the bright central region, potentially indicative of a more diffuse halo structure.
