The galaxy presents as a moderately bright, elliptical-like structure. The core region is considerably brighter and concentrated, with a yellowish hue indicative of an older stellar population. The light appears to fade gradually towards the outer regions. The overall shape is close to round, but with a subtle elongation. There is no obvious spiral arm structure or distinct dust lanes visible. There appear to be some small localized regions that show a slight color difference that might indicate a small amount of star formation is occurring, although this is low. There is no apparent major disturbance or merging features. The galaxy appears as a relatively isolated system.
