The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall shape is neither perfectly round nor elongated, appearing somewhere in between. There is a slight colour gradient, with the central region appearing more yellow/orange, suggesting a higher concentration of older stellar populations. Fainter blue regions indicate younger stars may be present. There is no obvious dust lane or spiral arm structure visible, and no signs of any major ongoing mergers or disturbances.
