The galaxy presents as a relatively small, somewhat smooth object. It exhibits a generally rounded morphology, with no obvious spiral arms or bar structure visible. The galaxy appears to have a bright central core that fades outward into a more diffuse halo. Based on the color profile, the core exhibits a bluer hue, suggesting younger stellar populations are more prominent here. The outer halo displays a redder color, which may indicate older stellar populations or dust obscuration. There are no evident signs of major mergers or tidal disturbances. Overall, the galaxy seems to be a relatively undisturbed system with ongoing but potentially low-level star formation.
