The galaxy presents as a relatively smooth, centrally concentrated object with a nearly circular morphology. A bright central region gradually diffuses outwards, lacking any prominent spiral arm structures or distinct features. The core exhibits a notably bright, concentrated luminosity, suggesting a significant stellar population and possible presence of an active galactic nucleus, though at this resolution it is impossible to confirm.

Colors appear fairly uniform across the galaxy, with a slight bluing towards the outer edges of the central concentration of the galaxy, potentially indicating some degree of ongoing star formation in the outer regions. The overall color suggests a fairly evolved stellar population, leaning toward older stars. There are no obvious signs of significant tidal interactions or recent merger events. The overall impression is that of a mature galaxy, likely an elliptical or S0 type, displaying a primarily smooth and uniform luminosity profile.
