The galaxy appears as a centrally concentrated, somewhat elliptical structure. The core region presents a bright, smooth appearance, suggesting a high density of stars, possibly an older stellar population. Moving outwards from the core, there is a gradual decrease in luminosity. Some faint, diffuse features are observable surrounding the core, perhaps indicating a weak disk or extended halo. There is a subtle color gradient, with a slight shift towards bluer hues in the outer regions, potentially indicative of ongoing star formation. The overall morphology appears relatively undisturbed, showing no signs of significant tidal interactions or major mergers, though subtle distortions can't be ruled out.
