The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellowish-orange hue, suggestive of an older stellar population. Fainter, diffuse bluish extensions emanate from the central region, potentially indicating regions of ongoing, albeit subdued, star formation. There is a hint of asymmetry in the outer regions, possibly due to minor tidal interactions or internal structures. The object lacks prominent spiral arms or a well-defined disk structure. Overall, the galaxy presents characteristics consistent with an evolved system that is transitioning to a red and dead spheroid.
