The galaxy presents a generally smooth, elliptical morphology. Its light profile appears relatively concentrated towards the center, suggesting an evolved stellar population. There is a subtle color gradient, with a slightly bluer hue in the outer regions, which could indicate some level of ongoing star formation, albeit at a relatively low rate. No prominent spiral arms or bar structures are discernible. The overall structure is somewhat rounded, without obvious signs of recent major merger activity, although there may be minor disturbances in the outskirts. The galaxy exhibits a reddish color index, typical of galaxies at intermediate redshifts. The estimated size corresponds to a galaxy of intermediate physical scale.
