The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge transitioning smoothly into an extended halo. The primary color is a warm, yellow-orange hue, suggesting a population dominated by older stars. There appears to be a lack of prominent spiral arms or dust lanes, which is consistent with the smooth classification. The galaxy appears relatively isolated with no obvious tidal features or nearby interacting companions observed in the field. Faint hints of a diffuse outer structure suggest the presence of a larger stellar halo, but this is difficult to ascertain with certainty. The overall roundness and lack of significant disturbance suggest that the galaxy has largely completed its morphological evolution.
