The galaxy presents as a relatively smooth, elliptical-like structure. It appears to lack prominent spiral arms or a well-defined disk. The central region exhibits a concentrated luminosity, suggesting a significant stellar population and potentially a central supermassive black hole. The light profile transitions smoothly from the core to the outer regions, with a gradual decrease in intensity. Faint, diffuse extensions are possibly present. The galaxy exhibits a color gradient, transitioning from a slightly redder hue at the center to a bluer tint in the outer regions, suggestive of differing stellar populations and ongoing star formation activity. There are no obvious signs of major ongoing mergers or significant tidal disturbances, although subtle asymmetry or faint, disturbed features cannot be entirely ruled out.
