The galaxy presents an elliptical morphology, appearing mostly smooth and featureless. The core is a bright yellowish-white, suggesting a high concentration of older stellar populations. Moving outwards from the core, the galaxy exhibits a gradual decrease in luminosity. The outer regions display a reddish-brown hue, possibly indicating the presence of a lower density of younger, bluer stars, or the presence of dust. There's no visible spiral arm structure or prominent dust lanes. Overall, the galaxy appears to be relatively undisturbed, without evidence of ongoing mergers or significant tidal interactions. It appears to be a moderately sized galaxy.
