This galaxy appears to be a relatively compact system, estimated to be approximately 8 arcseconds in diameter. It exhibits a flattened, disk-like structure, viewed at an angle that suggests it is likely a spiral or lenticular galaxy. The central region of the galaxy is notably bright, exhibiting a concentrated luminosity profile, which suggests a bulge component. The overall color of the galaxy appears to be slightly redder, indicating an older stellar population. Faint, asymmetric features suggest a minor disturbance, possibly due to a recent minor merger.
