The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a yellowish hue, suggesting a stellar population dominated by older, evolved stars and a relative paucity of ongoing star formation. The isophotes appear largely regular and undisturbed. There is no visible spiral arm structure or significant dust lane obscuration. The object appears neither particularly round nor elongated but rather intermediate in apparent shape. There is no strong evidence of tidal features or ongoing merger activity. The galaxy's light profile seems to fade gradually from the core, indicating a lack of sharp boundaries.
