The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge is evident, exhibiting a yellowish hue, suggestive of an older stellar population. The light fades gradually from the central bulge outwards, with minimal discernible disk features. The overall round shape with a smooth light distribution, hints at a relatively quiescent galaxy, possibly in a more evolved stage of its evolution, with little to no ongoing major merging events currently disrupting its structure.
