The galaxy presents as a disk-type galaxy, observed nearly edge-on from our vantage point. There is a prominent central bulge, characterized by a smooth, concentrated luminosity profile. The disk itself appears relatively thin and extended. There is dust visible in the disk. It is visible as darker splotches. Indications of potential tidal features, such as faint extensions or asymmetries in the disk's outer regions, suggest the galaxy might be undergoing or have undergone a gravitational interaction with another galaxy. The color suggests older stars are present. The galaxy exhibits a faint bluish color in the outer regions which may point to younger stars in the disk. The galaxy's overall structure implies a complex evolutionary history, potentially shaped by mergers or accretion events. It may be forming stars at a lower rate.
