The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round. There is no apparent indication of a pronounced disk structure or spiral arms. A slight color gradient can be observed, with a suggestion of a bluer hue towards the central region of the galaxy, potentially indicating a concentration of younger stellar populations there. No obvious signs of tidal disturbances, major mergers, or significant ongoing star formation are readily apparent.
