The galaxy presents as a generally smooth, centrally concentrated object with a high degree of radial symmetry. It exhibits a round morphology, lacking any discernible spiral arms or bar-like features. The light distribution is centrally dominant, with a bright core region that gradually diminishes in intensity towards the outer edges. There are no apparent major distortions or tidal tails indicative of recent major merger activity, though minor disturbances cannot be ruled out at this resolution. The color appears relatively homogenous across the galaxy, with a slight reddening towards the core and bluer tints towards the outer regions, suggesting the presence of older stellar populations in the central bulge and the possibility of some ongoing, though low-level, star formation in the outer regions. The overall appearance is consistent with an elliptical galaxy or a lenticular galaxy viewed face-on. The galaxy appears to be a significant distance away from us.
