The galaxy presents as a somewhat elongated, elliptical structure. It appears largely smooth in texture, with a concentrated central bulge that exhibits a yellowish-white hue, likely indicating an older stellar population. A faint, diffuse disk component can be inferred, displaying a subtle bluish tint towards the outer edges, potentially indicative of ongoing or recent star formation activity, albeit at a relatively low rate. The galaxy does not exhibit any obvious signs of spiral arms or significant morphological disturbances, such as tidal tails or distortions, suggesting it is not currently undergoing a major merger event. However, a minor irregularity or asymmetry in the outer regions cannot be completely ruled out based on the image resolution. The overall morphology points towards a galaxy that has largely exhausted its gas supply and has settled into a more quiescent state.
