This galaxy exhibits a morphology that suggests an elliptical or lenticular classification. The central region presents a high concentration of luminosity, appearing mostly smooth and round. The light distribution shows a gradual decrease in intensity from the center towards the outer regions. There is evidence of a slight asymmetry or disturbance, possibly indicating minor tidal interactions or a recent minor merger event. However, a significant portion of its structure remains largely undisturbed. Color gradients suggest varying stellar populations or dust content throughout the galaxy. Specifically, the central bulge appears to have a yellowish hue, possibly from older stars. The outer regions show a slightly bluer tint, which may be due to some younger stellar populations. Overall, it presents a morphology consistent with a galaxy undergoing a relatively quiet evolutionary stage.
