The galaxy presents as a single, relatively concentrated object with a smooth appearance. Its central region exhibits a yellowish hue, suggesting an older stellar population. A bluer, more diffuse halo surrounds this core, indicating the presence of younger stars and possibly some ongoing star formation. The overall structure is somewhat elliptical, with no clear evidence of spiral arms or a prominent disk. There appear to be minor disturbances in the outer regions of the halo, though the nature of these are unclear. They could be the remnants of a minor merger, tidal streams, or simply irregularities in the gas distribution. There is no visible central bar structure. The image is consistent with a relatively massive galaxy, possibly a lenticular or early-type spiral.
