The galaxy presents as a flattened, elliptical morphology, exhibiting a smooth light distribution across its surface. It displays a concentrated central bulge that transitions into a faint, extended disk. Color gradients suggest a centrally concentrated population of older stars, indicated by the yellower hue of the core, with a bluer population of younger stars present in the outer regions of the disk, which implies some amount of ongoing star formation. There are subtle signs of disturbance within the disk, potentially indicating a past or ongoing interaction or minor merger event. Overall, the galaxy appears relatively undisturbed with only mild irregularities, indicating it is likely undergoing quiescent evolution.
