The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology and a centrally concentrated luminosity profile. It exhibits a yellowish-white hue in its central region, indicating an older stellar population with lower rates of star formation. A faint redder ring appears to surround the central region, potentially indicating regions of dust and ongoing or recent star formation, albeit at a relatively low level. The galaxy is observed to have an intermediate ellipticity, appearing somewhat elongated. No signs of tidal tails, bridges, or other major disturbances are apparent, suggesting it is unlikely to be undergoing a major merger event.
