The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated core. There is a noticeable falloff in luminosity from the center outwards, resulting in a diffuse halo. The overall color profile suggests an older stellar population, with a yellowish hue dominating the central region, transitioning to a redder color as we move outward. It appears predominantly undisturbed, with no obvious signs of recent major mergers or strong tidal interactions. There may be minor irregularities in the outer regions, suggesting minor past interactions. The morphology is generally well-defined, with a moderately rounded shape, but lacks defined spiral arms or a prominent disk structure.
