The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, surrounded by a more diffuse halo. The color gradient transitions from a yellowish hue in the core to a redder color towards the outer regions, suggesting an older stellar population in the outer parts of the galaxy. There is no visible evidence of spiral arms or significant dust lanes. The overall shape is elongated, exhibiting a noticeable ellipticity, with a major axis that appears roughly twice the length of the minor axis. There are no obvious signs of ongoing mergers or tidal disturbances.
