The galaxy presents as a relatively compact, centrally concentrated object. The light profile appears smooth and diffuse, lacking distinct spiral arm structures or a prominent bar. The galaxy exhibits a generally elliptical morphology, appearing mostly 'in between' round and elliptical. There is no strong evidence of significant dust lanes or recent major merger activity. Faint and subtle tidal features or minor disturbances are not ruled out. The overall color is a subdued yellowish-white, suggesting a stellar population dominated by older, less massive stars. The presence of minimal star formation is inferred from the relatively passive color. The estimated size is likely on the smaller end for galaxies.
