This galaxy exhibits a predominantly smooth morphology with a somewhat elongated shape. It displays a central bulge that appears relatively bright and concentrated. The overall color gradient suggests an older stellar population, particularly within the bulge. A faint disk-like structure is hinted at, displaying a bluer hue in the surrounding regions, which may be due to lower levels of star formation. No major disturbances or tidal features are discernible, indicating it is likely not undergoing a major merger event.
