The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light profile exhibits a radial gradient, being brightest at the core and gradually diminishing outward, suggesting a smooth distribution of stars within the galaxy. There's a slight elongation to the galaxy's shape. No distinct spiral arms or prominent dust lanes are readily apparent in the observed visible light, indicating the galaxy is likely a more evolved system with little active star formation. The color index suggests an older stellar population, leaning towards redder wavelengths. It shows a relatively undisturbed morphology. There is no evidence to indicate ongoing major or minor mergers.
