The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The core exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outwards from the core, the galaxy displays a gradual decrease in surface brightness. There is some indication of faint, diffuse outer regions, exhibiting a bluer color possibly related to the presence of a younger population of stars, although star formation appears to be relatively low. There is a slight hint of a disturbance in the structure, but no clear indications of significant merging activity or tidal features. The overall shape appears close to circular, suggesting a minimal degree of rotational support.
