The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated, bright central bulge. The overall color appears yellow-orange, suggesting a population of older stars with lower rates of on-going star formation. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a round shape, lacking a prominent disk-like structure. No signs of major merging events or tidal disturbances are immediately apparent, although some minor irregularities in the outer regions cannot be ruled out. The galaxy has a diameter of around 5 kpc.
