The galaxy presents an elliptical morphology with a prominent central bulge. The core exhibits high luminosity, suggesting a concentration of stars and possibly an active galactic nucleus. Fainter extended halos are seen around the galaxy. The texture of the galaxy appears relatively smooth, with limited evidence of significant spiral arm structure or distinct dust lanes. There is very little evidence of merging or tidal disturbance. There is a general yellow-white hue, but the presence of some slightly bluer regions may indicate pockets of younger star formation.
