The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellow-orange hue, potentially indicative of an older stellar population. The isophotes appear generally round, with a slight elongation. No distinct spiral arms or prominent dust lanes are discernible in the image. There are hints of a faint, diffuse halo surrounding the central region, with a subtle blueish tint, suggesting the presence of some younger stars. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent major merger activity or strong tidal interactions. The galaxy has a low rate of star formation.
