The galaxy presents as a flattened, elliptical shape, displaying a smooth morphology with a general lack of discernible features such as spiral arms. The light distribution appears concentrated towards the center, indicating a possible bulge. The color gradient suggests older stellar populations dominate, emitting redder light. The galaxy exhibits a slight elongation, appearing somewhere between round and cigar-shaped. There is some evidence of tidal disturbance. These may be minor features, but it is possible that the galaxy is currently undergoing a slow merger. The galaxy has a moderate mass and a low star formation rate.
