The galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a yellowish-white hue, indicative of an older stellar population. Moving outward from the core, a faint greenish-blue halo is observed. The galaxy appears slightly elliptical. No prominent spiral arms or bar structures are discernible. There may be minor disturbances but not significant enough to say that the galaxy is merging. The overall morphology is consistent with an early-type galaxy.
