The galaxy presents a largely smooth and concentrated morphology. It appears elliptical in shape, with a high degree of central concentration. The galaxy's light profile exhibits a radial gradient, increasing in brightness towards a very bright core. 

There is no strong evidence of spiral arms or a prominent disk component. Faint bluish colorations are observed in the outer regions, suggestive of some ongoing star formation, albeit at a low level. The galaxy appears relatively undisturbed, lacking the visual signatures of recent major mergers or tidal interactions. Subtle irregularities may be present, but the overall structure remains largely regular and symmetrical.
