The galaxy appears to be a relatively luminous system, exhibiting a central concentration of light with a somewhat diffuse and extended halo. Morphologically, it appears to be largely elliptical, with a smooth, rounded shape. There is a subtle hint of a disk-like structure, though the lack of prominent spiral arms suggests it may be a lenticular or early-type spiral galaxy. The color index indicates a redder overall population, suggesting a relatively older stellar population and suppressed star formation. Faint, possibly tidal features, hint that the galaxy may have undergone minor merger event.