The galaxy presents an elliptical morphology with a smooth texture, exhibiting a concentrated central bulge which emanates a yellowish hue, possibly indicating an older stellar population. A faint, disk-like structure surrounds the central bulge. The structure is elongated, appearing moderately inclined to our line of sight. There are no obvious spiral arms or distinct dust lanes visible. The outer regions of the galaxy gradually fade into the background sky. Overall, the galaxy gives the impression of being a relatively undisturbed system, lacking signs of recent major mergers or active star formation.
