The galaxy appears as a lenticular, disk-shaped system, viewed at an oblique angle. There is a noticeable bulge that seems to be the brightest part of the galaxy. A faint disk extends beyond the bulge, exhibiting a smoother texture with no apparent spiral arm structure. The disk displays a generally yellowish-white color, suggestive of an older stellar population. Overall, the galaxy appears to be relatively undisturbed, without significant signs of ongoing mergers or tidal interactions. The morphology suggests a system that has largely exhausted its gas reservoir and undergone significant bulge growth.
