The galaxy presents a largely smooth and elliptical morphology. The core region exhibits a high degree of luminosity, suggesting a concentrated stellar population. The overall color appears to be on the redder end of the spectrum. There's little evidence of significant spiral arm structure or dust lanes. The shape is somewhat oval, and the outer regions exhibit a relatively gradual decrease in luminosity. The image shows no major signs of ongoing mergers, tidal tails, or significant morphological disturbances. There may be a subtle asymmetry, but the galaxy appears largely undisturbed.
