The galaxy presents a generally elliptical morphology, with a smooth, diffuse light distribution. The central region exhibits a yellowish-white hue, suggesting a relatively older stellar population. Towards the outer edges, a faint bluish tint is observed, potentially indicating the presence of some younger, hotter stars or ongoing, although limited, star formation within the galaxy's disk. The galaxy appears to be undergoing only minor disturbances, likely due to gravitational interactions or internal dynamics. The galaxy's shape appears more in between round and cigar shaped, leaning more towards round. The light profile suggests a concentrated bulge. The overall impression is that of a lenticular or early-type spiral galaxy undergoing a period of relative quiescence.
