The galaxy appears as a relatively smooth, elliptical object, exhibiting a high degree of central concentration of light. The core region is bright and appears nearly circular with a slight elongation. A gradual fading of intensity is observed moving outward from the center, with no apparent substructure such as spiral arms or a distinct bar. The galaxy presents an almost uniform color profile, indicating an older stellar population and minimal ongoing star formation activity. There is no visual indication of any major disturbances, such as tidal tails or ongoing merger activity, and it appears to be a settled system. Overall, the galaxy is compact and has a high Sersic index, which indicates the galaxy is more concentrated, similar to an elliptical galaxy.
