The galaxy presents a largely smooth and rounded morphology. It exhibits a concentrated central bulge that appears quite luminous, with a gradual decrease in surface brightness extending outwards. The galaxy has an elliptical shape, with the isophotes appearing almost circular. The color gradient suggests that the central regions may be dominated by older stellar populations, while the outer regions may exhibit a slightly bluer hue, potentially indicating some younger stars or a small amount of on-going star formation. No distinct spiral arms or bar structures are discernible. There is a slight hint of disturbance in the galaxy's overall shape, perhaps the result of a minor interaction. There is a small amount of tidal debris present in the galaxy's halo.
