The galaxy presents as a relatively smooth and centrally concentrated structure. It appears elliptical in shape, with a high degree of symmetry. There is no obvious spiral arm structure or bar visible. The central region exhibits a bright, concentrated core, likely indicative of a galactic nucleus.

The color gradient suggests a relatively old stellar population, although there may be a small degree of on-going star formation. The overall color is moderately red, which would typically indicate evolved stars, and there may be some younger, bluer stars in the galaxy. There is no evidence of strong tidal disturbances or merging activity.
