The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, presenting a rounded appearance with no obvious spiral arm structures or strong bar features. A bright central bulge dominates the luminosity profile, indicating a concentration of older stars and a likely supermassive black hole at the nucleus.

A faint, diffuse halo surrounds the central region, subtly extending the galaxy's overall size. There is a slight color gradient observable; the central bulge appears whiter, potentially indicative of an older stellar population, with the outer regions showing a hint of bluer coloration, suggesting the presence of younger stars.

No significant signs of ongoing merger activity, such as tidal tails or distorted morphologies, are apparent. The galaxy seems to be relatively undisturbed, existing as an isolated system or potentially interacting with companions too distant or faint to be detected in this image.
