The galaxy presents as a slightly elongated, lenticular structure with a smooth, concentrated central bulge exhibiting a yellowish hue. A fainter, bluer disk surrounds the bulge, indicating the presence of a younger stellar population in the outer regions. The overall morphology suggests a system undergoing, or having completed, a transition from a spiral-dominated to a more elliptical-like form. There is a slight asymmetry observed in the outer disk region, potentially indicative of a minor interaction or past merger event. Star formation is likely ongoing, albeit at a relatively low rate, primarily within the disk component. The galaxy appears relatively isolated, showing no immediate signs of major ongoing mergers or tidal disruptions.
