The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, symmetrical structure. There is no visible evidence of spiral arms or a prominent disk. The light distribution is concentrated towards the center, with a gradual decrease in luminosity outward. The core region presents a yellowish-orange hue, possibly indicating an older stellar population dominated by evolved stars. There is a slight color gradient moving outwards, potentially indicating younger, bluer stars present in the galaxy's halo. It shows no signs of any major interaction or disturbances from mergers. The general morphology of the galaxy suggests a relatively relaxed system in a later stage of evolution.
