The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. It appears elliptical in shape, though not perfectly round; there is a slight elongation. The galaxy's color profile indicates an older stellar population, dominated by redder hues in the central bulge, transitioning subtly to slightly bluer colors at the outer edges of the galactic halo. The core region displays a very high luminosity. There is no obvious presence of significant spiral arm structures or a prominent disk. There are subtle indications of minor disturbances or asymmetries in the outer regions, but no clear evidence of ongoing major mergers or strong tidal interactions. Overall, the galaxy presents a somewhat undisturbed, evolved system.
