The galaxy presents as a largely featureless elliptical or lenticular system, with a dominant smooth morphology. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness outward from the core. The overall color is relatively uniform, trending towards a yellow-red hue, suggesting a stellar population dominated by older, redder stars and a low rate of ongoing star formation. No distinct spiral arm structures or prominent dust lanes are discernible within the available image resolution. The isophotes appear generally regular, with a mild deviation from perfect circularity. There are no obvious signs of a major ongoing merger, although a minor tidal interaction or past merger event cannot be ruled out based solely on this image.
