The galaxy presents a fairly smooth, elliptical morphology, appearing somewhat rounded in shape. There is a central concentration of light that is bright and slightly blue-shifted, suggestive of possible star formation or an active galactic nucleus. The galaxy appears to be relatively isolated with no strong signs of major mergers or tidal disturbances, but there is a slight asymmetry suggesting a possible minor interaction or disturbance. The outer regions fade gradually into the background sky. The galaxy has a discernible color gradient, shifting towards a redder hue in the outer regions, which could be indicative of an older stellar population in the outer regions.
