The galaxy exhibits a smooth, elliptical morphology with a high Sersic index, suggesting it is a spheroidal galaxy. The light distribution appears highly concentrated towards the center, with a rapid decrease in surface brightness towards the outer regions. The color profile indicates a relatively red galaxy, suggesting an older stellar population and reduced star formation activity. There is a slight flattening observed, but the galaxy is mostly circular. There is little to no evidence of spiral arms, dust lanes, or other features associated with disk galaxies. The galaxy appears relatively undisturbed, with no obvious signs of recent mergers or tidal interactions. The estimated size is approximately 4.4 kpc in radius. Overall, it presents the appearance of a mature, passively evolving galaxy.
