The galaxy presents as a lenticular or early-type spiral galaxy, seen at an oblique angle. There is a prominent central bulge that appears nearly spheroidal, exhibiting a bright, concentrated luminosity gradient towards the core. Fainter, more diffuse structures extending outwards from the central bulge suggest the presence of a disk component. The disk seems relatively smooth, with a gradual decrease in surface brightness from the inner regions to the outer edges. There's a suggestion of faint spiral arms. Overall, the galaxy appears relatively undisturbed, without any obvious signs of major mergers or tidal interactions. The colors observed are consistent with an older stellar population, with a yellowish/reddish hue dominating the light emitted.