The galaxy presents a generally smooth morphology with a near-perfectly round shape. A concentrated central bulge region dominates the light profile, appearing with a distinct reddish-orange hue. This suggests a population of older stars concentrated in the galactic center. Surrounding the bulge, a fainter, more diffuse disk-like structure is visible with a faint greenish tinge. The lack of distinct spiral arm features or significant dust lanes indicates it is likely an early-type galaxy, such as an elliptical or lenticular galaxy, but with a hint of ongoing, albeit low, star formation activity in its outer regions. There is no evidence of major mergers or significant tidal disturbances in its structure. Faint irregularities hint at the presence of minor disturbances, but its general appearance is that of a relaxed and relatively undisturbed system. Overall, the galaxy presents characteristics of an evolved galaxy with a dominant old stellar population, but with low levels of recent star formation.
