The galaxy presents a largely smooth, elliptical morphology. The light distribution is concentrated towards the center, with a gradual decrease in surface brightness outwards. There is a distinct lack of resolved spiral arms or prominent dust lanes, suggesting a relatively evolved system. The galaxy exhibits an elongated shape, with the major axis oriented approximately northeast to southwest. Color gradients appear subtle, with a slightly bluer hue towards the outer regions compared to the yellowish core, possibly indicative of ongoing, but weak, star formation at the edges. Overall, the galaxy appears to be a relatively quiescent elliptical, lacking major disturbances or signs of recent merger activity.
