The galaxy presents as a relatively smooth, elliptical-like structure. The color profile indicates a dominant yellowish-orange hue centrally, suggesting an older stellar population. There is a subtle color gradient, transitioning towards a redder periphery, which would be consistent with a population of cooler, older stars towards the outer regions. The overall morphology appears undisturbed, without any obvious signs of tidal tails, asymmetric features, or ongoing major mergers. It appears relatively isolated. The object exhibits a high degree of central concentration, with a gradual decrease in surface brightness moving outwards.
