The galaxy presents as a disk-shaped system, with a moderately bright, concentrated central bulge exhibiting a yellowish hue. The disk component appears relatively smooth and featureless, lacking prominent spiral arms or dust lanes discernible at this resolution. The overall color gradient suggests a population of older stars dominating the central bulge, with potentially younger, bluer stars contributing to the disk's luminosity. The galaxy's ellipticity indicates it is viewed at a moderate inclination. There are no obvious signs of strong tidal interactions or major mergers, although a minor disturbance or interaction cannot be ruled out given the smoothness of the disk. The overall morphology points towards an intermediate-type spiral or a lenticular galaxy.
