This galaxy exhibits a clear disk morphology, viewed nearly edge-on. A prominent bulge, appearing somewhat rounded, dominates the central region. There is a slight indication of dust lane obscuration along the plane of the disk, contributing to the galaxy's overall redder appearance. The disk itself is relatively thin. The system shows no immediately obvious signs of major mergers or significant tidal disturbances, although minor irregularities are present in the disk. The overall color suggests a evolved stellar population, potentially indicating a modest star formation rate.
