The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions into a more diffuse halo. The color gradient suggests a concentration of older stellar populations within the central region, indicated by the yellower hue. Fainter, bluer colors in the outer regions hint at the possibility of some younger stars, though the limited resolution makes a definitive assessment difficult. There is a slight elongation observed, moving from the upper left of the galaxy to the lower right. There are no obvious spiral arm structures or significant dust lane features visible. The overall smooth appearance suggests this galaxy is likely to have undergone, or is currently undergoing, relatively little active star formation.
