The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white glow, indicating a high density of stars or a possible active galactic nucleus. The light gradually diminishes outwards from the core in a fairly symmetrical manner. The overall color is slightly redder than the core, suggesting an older stellar population in the outer regions. There may be a faint disk-like structure or residual tidal features, however the smooth appearance dominates. There are no apparent distinct spiral arms or irregular structures. The galaxy appears relatively undisturbed, showing no strong evidence of recent major mergers or interactions.
