The galaxy presents a primarily smooth morphology, exhibiting minimal apparent substructure. It appears elliptical in shape, closely approaching a circular form. The central region displays a high degree of concentration with light gradually diminishing toward the outer regions. The light from the galaxy has a redder color, which may indicate the presence of an older stellar population. There are no visual indications of spiral arms or a prominent disk component. The overall appearance suggests the galaxy is relatively undisturbed, without any significant signs of tidal interactions or major mergers.
