The galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and symmetrical morphology. It is highly concentrated, with a bright central bulge that gradually fades towards the outer edges. There is no visible evidence of spiral arms or a disk-like structure. The galaxy displays a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of current star formation. The overall structure does not indicate any significant recent or ongoing mergers or tidal disturbances. Its round shape indicates a lack of rotation. 
