This galaxy appears to be a relatively smooth, disk-like system, viewed at a considerable angle. The central bulge is prominent, exhibiting a high surface brightness and a yellowish-white color, suggesting a population of older stars. Extending outward from the bulge is a fainter, flattened disk component. Subtle variations in color are present within the disk; some regions are slightly bluer, hinting at the presence of younger stars and ongoing star formation, however, the overall color indicates that it is a primarily older stellar population. There is little to no evidence of strong spiral arm structure. The overall shape is elliptical, indicating it might be an intermediate-type spiral or a lenticular galaxy. The edges of the disk fade gradually into the background, with no sharp truncation observed. The symmetry of the galaxy is relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. There is possibly minor disturbances.
