The galaxy presents a relatively smooth, elliptical morphology. There is some indication of minor internal structure, but no obvious spiral arms or a prominent disk. The galaxy appears to be largely spheroidal in shape, with an approximate effective radius of 5.5 kpc. Color gradients within the galaxy are subtle, with a generally redder core region and a slightly bluer outer halo, potentially indicative of older stellar populations concentrated towards the center and younger stars in the outer regions. The image shows no signs of major mergers or tidal disturbances, and the galaxy exhibits a fairly regular shape. The galaxy has an estimated stellar mass on the order of 10^11 solar masses and a low star formation rate. Overall, the galaxy seems to be a fairly relaxed system, likely an elliptical galaxy with a quiescent star formation history.
