This galaxy appears to be a relatively compact elliptical galaxy. Its light profile is smooth and concentrated, with a centrally peaked brightness distribution and a gradual decline in intensity outward. The overall color is yellowish-orange, suggesting an older stellar population that is dominated by redder giant stars. There is no clear evidence of spiral arms, a disk-like structure, or significant dust lanes. The galaxy is generally round in appearance, showing no signs of major disturbances or ongoing mergers, although subtle asymmetries are possibly present. Based on the color and apparent lack of star formation indicators, this galaxy likely has a low star formation rate and specific star formation rate. The estimated size suggests this is a galaxy of intermediate scale.
