The galaxy presents as a largely smooth, elliptical object with a concentrated central bulge. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. The outer regions display a gradual decrease in luminosity, transitioning to a reddish-orange color. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively isolated, with no signs of major interactions or mergers, although there are some slight irregularities in the outer isophotes. The overall morphology suggests an evolved system, likely a massive elliptical galaxy at a moderate redshift. The estimated size indicates a substantial physical extent. Its color profile is consistent with a population of older stars and a relatively low star formation rate.
