The galaxy presents a primarily smooth, elliptical morphology. It exhibits a centrally concentrated bulge with a gradual decrease in surface brightness towards its outer regions. The overall shape appears largely circular, with a slight deviation toward a more elongated form. There is no clear evidence of prominent spiral arms or a distinct disk structure. The galaxy's color profile is dominated by yellow and red hues, suggesting a stellar population that is relatively old and metal-rich. There is no indication of significant dust lanes or recent star formation activity based on the absence of blue or UV emission. Subtle irregularities in the galaxy's halo might indicate minor gravitational interactions.
