The galaxy appears to be a relatively smooth, centrally concentrated system. The light profile suggests an elliptical morphology, though there is a slight flattening. The central region is bright and concentrated, with a gradual falloff in surface brightness moving outward. The color appears slightly redder in the central region, transitioning to a bluer hue in the outer regions, which may indicate ongoing or recent star formation in the outer disk. A smaller, irregular, possibly tidally distorted feature is located nearby that may be interacting with the central system.
