The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. It exhibits a yellowish-orange hue, suggesting a population dominated by older stars. There's a noticeable lack of distinct spiral arms or dust lanes, further reinforcing the elliptical classification. The galaxy appears relatively isolated with no obvious signs of major tidal disturbances or ongoing mergers, although some minor asymmetry cannot be ruled out. The overall light distribution is centrally concentrated, fading gradually outwards with a somewhat diffuse boundary.
