The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated, bright core that gradually fades into the outer regions, displaying a diffuse halo. The overall color appears yellowish, suggesting an older stellar population with a lower rate of ongoing star formation. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears to be isolated, without any obvious signs of tidal interactions or major disturbances indicative of recent mergers, though a slight asymmetry in the outer halo might suggest minor disturbances.
