The galaxy appears as a centrally concentrated object with a predominantly smooth morphology. It exhibits a near-elliptical shape, displaying a high degree of central light concentration that appears to fall off radially towards the edges. The galaxy's colour profile indicates a predominantly yellow hue at the nucleus and inner regions, suggesting an older stellar population. The outer regions display a subtle bluer tint that may indicate some degree of ongoing or recent star formation but not in a strong manner. There is no evidence of spiral arm structure, a prominent disk, or major disturbances indicating a major merger event. Minor structural asymmetry may be present, which could be a hint of past interactions or minor mergers. The galaxy shows an apparent regular structure indicative of a system that has undergone a reasonable amount of gravitational relaxation.
