The galaxy presents as a slightly elongated spheroid, exhibiting a smooth, diffuse light profile suggestive of an elliptical galaxy. The central region is brighter, with a gradual decrease in luminosity towards the outer edges. The overall color appears yellowish-orange, implying a stellar population dominated by older, cooler stars. There is no obvious evidence of spiral arm structure, dust lanes, or active star-forming regions. The galaxy does not display any signs of significant tidal disturbances or ongoing mergers, though there is some slight irregularity on the edges suggesting some sort of interaction.
