The galaxy presents an elliptical morphology. It exhibits a smooth, centralized light distribution, suggesting a lack of significant spiral arm structure or prominent dust lanes. The galaxy's color appears largely uniform, with a subtle shift toward redder hues, implying an older stellar population. It has a generally rounded shape, with only slight deviations from a perfect circle. There is no visual evidence of ongoing major mergers or significant tidal disturbances, although subtle irregularities may be present. The galaxy's compactness suggests a relatively high stellar density.
