The galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless structure. It displays a somewhat rounded shape, though slightly elongated along one axis. There is no discernible spiral arm structure or prominent dust lanes visible. The galaxy's light distribution is centrally concentrated, with a gradual decrease in intensity towards its outer edges. Color gradients suggest a higher concentration of older stellar populations within the central regions, manifesting as a slightly redder hue compared to the bluer, albeit faint, outer regions. There is a possible, very minor disturbance in the galaxy's overall shape, though this could also be due to image resolution limitations. Overall, the galaxy appears to be a quiescent system with a low star formation rate.
