The galaxy appears to be a luminous, relatively smooth object. Its morphology suggests a significant spheroidal component. The light distribution is centrally concentrated with a noticeable falloff in intensity towards the outer regions. The main body exhibits an elliptical shape, appearing nearly circular with a slight elongation. There is little evidence of spiral arms or distinct disk features.

The galaxy's color appears to be yellowish-white, suggesting a population of older stars. There are no prominent blue regions indicative of ongoing, significant star formation. There is a hint of a very faint, diffuse structure extending slightly beyond the main body of the galaxy, which may represent a stellar halo or the remnants of past interactions. There are no obvious signs of major mergers or tidal disruptions in the immediate vicinity, and the galaxy appears relatively undisturbed.
