The galaxy appears as an elliptical-like structure with a bright, concentrated central bulge that transitions smoothly outwards. The core region exhibits a yellowish-white hue, suggesting a population of older stars. The outer regions display a slightly bluer tint, possibly indicating the presence of younger stellar populations or ongoing star formation. There is a general smoothness to the galaxy's appearance, with only subtle deviations from a perfectly elliptical shape. Faint irregularities around the central bulge may suggest that the galaxy is in the process of a minor disturbance. Overall, the galaxy seems to be in a fairly settled state, without clear indications of major recent merger activity.
