The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy, viewed at an oblique angle. It exhibits a bright, concentrated central bulge that dominates its overall luminosity. The bulge shows a yellow to slightly orange hue, suggestive of an older stellar population. A faint, bluish disk component is discernible extending outwards from the bulge, indicating some ongoing, though subdued, star formation. This disk does not show any well-defined spiral arm structure but appears generally amorphous with slight clumpy regions on the periphery. The overall shape is roughly elliptical, with an intermediate roundness, and a cigar-shaped form cannot be excluded. There is no strong evidence of any ongoing major mergers or significant tidal disturbances affecting the system. There are some suggestions of minor disturbances in the disk.
