The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light distribution. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. Moving outward, the color gradually transitions to a more reddish-orange tint within the galaxy's extended halo. There appears to be a slight asymmetry in the outer regions with some faint indication of a possible tidal feature or minor disturbance on one side. There is no visible evidence of prominent spiral arms or significant dust lanes. The overall roundness of the galaxy indicates it is likely viewed close to face-on. There is no sign of active star formation within the galaxy.
