The galaxy presents as a mildly elliptical structure with a smooth, diffuse morphology. A central bulge region exhibits a reddish hue, potentially indicating a population of older stars. Moving outward from the bulge, the disk appears bluer, suggesting ongoing or recent star formation. The galaxy appears to be relatively undisturbed with no strong signs of tidal interactions or major mergers; although, there are mild disturbances present. The overall smoothness suggests a mature system, potentially in transition toward a more quiescent state.
