The galaxy appears as a single, relatively smooth object with an elliptical morphology. The light distribution is centrally concentrated, characterized by a bright core. The color profile suggests an older stellar population dominating the light output. Specifically, the galaxy exhibits a yellow-red hue indicating a lack of significant recent star formation. There is no visible disk or spiral arm structure, nor is there evidence of any significant tidal disturbances or ongoing merger activity. Based on the smoothness of the profile, it is likely an early-type galaxy.
