The galaxy presents an overall elliptical morphology, with a smooth, centrally concentrated bulge. The light distribution suggests a primarily older stellar population dominating the core region, indicated by the yellowish hue. There is some evidence of bluer light on one side, suggesting the potential for regions of ongoing star formation. There appear to be faint extensions or tidal features, possibly indicative of past or ongoing gravitational interactions, or minor disturbances, but the resolution makes definitive identification difficult. The galaxy appears fairly luminous, suggesting a significant stellar mass, and likely resides at a considerable distance.
