The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. It appears elliptical in shape, with the major axis oriented vertically in the image. The light profile suggests a bulge-dominated structure, characterized by a bright, compact nucleus that gradually fades into the surrounding halo. Color gradients are subtly visible. The core region presents a yellowish hue, possibly indicative of an older stellar population. Moving outward, the color becomes slightly bluer, potentially suggesting the presence of some younger stars, albeit at a low rate of formation. There are slight asymmetries visible in the outer regions of the galaxy suggesting minor interactions with smaller galaxies, but the overall structure is still relatively undisturbed. 
