The galaxy presents as a centrally concentrated object with a smooth, diffuse profile. Its overall shape is elliptical, appearing elongated in the horizontal axis. The light distribution is not uniform, with a brighter, yellowish core region that gradually fades towards the edges. There is no discernible spiral arm structure or dust lane visible. The color gradient suggests a population of older stars, with a possible indication of ongoing low-level star formation, particularly in the central region. There are no signs of significant tidal disturbances or merging activity, and the overall morphology suggests a relatively undisturbed system.
