The galaxy exhibits a generally smooth morphology, appearing as a single, relatively undisturbed structure. The central region displays a concentrated, bright core, possibly indicative of an active galactic nucleus or a dense stellar population. The overall shape tends towards elliptical or spheroidal, with a moderate ellipticity, lacking any prominent spiral arms or disk-like features. Color gradients are present, with a reddish-yellow hue dominating the central regions, transitioning to bluer tones towards the periphery. This may suggest older stellar populations concentrated centrally, with younger, bluer stars more dispersed in the outer regions. There's a subtle suggestion of minor structural asymmetry, indicating possible past interactions or internal dynamics.
