The galaxy presents as a somewhat elongated, elliptical structure. It appears to possess a centrally concentrated bulge that transitions smoothly into a more diffuse halo. The color gradient suggests a population of older stars dominating the bulge region. The outer regions of the galaxy exhibit a bluer hue, possibly indicative of ongoing or recent star formation within a relatively faint disk component. No distinct spiral arms or prominent dust lanes are discernible in the image. The overall morphology appears relatively undisturbed, without obvious signs of tidal interactions or major mergers, though minor disturbances cannot be ruled out at this resolution. The galaxy's smooth, concentrated light profile and color characteristics are suggestive of a galaxy that is in the process of evolving from star-forming to a more passive state.
