The galaxy appears to be a spiral type, exhibiting a central bulge region that transitions into a more diffuse disk. Faint spiral arm structures are discernable, winding outwards from the central bulge. These spiral arms show some patchiness, which may indicate areas of active star formation. The disk is not perfectly symmetrical, which suggests the possibility of tidal interactions or a recent merger event. There is a weak bar-like structure visible in the center. The overall color gradient suggests an older stellar population in the bulge, gradually giving way to younger, bluer stars in the disk and spiral arms. The size of the central bulge relative to the entire galaxy appears to be moderate. The galaxy appears to be in a relatively undisturbed state.