The galaxy presents as a slightly elongated, lenticular structure with a prominent central bulge. The light distribution appears smooth and relatively featureless, suggesting an older stellar population. There's no apparent spiral arm structure or dust lanes visible in the image. The galaxy exhibits a color gradient, transitioning from a yellowish-white hue in the central region to a bluer tint in the outer regions, indicative of potential differences in stellar composition or age. The outskirts of the galaxy are diffuse and appear to gradually fade into the background. There is no evidence of any major disturbances or ongoing mergers.
