The galaxy presents a smooth, elliptical morphology. There is a lack of discernible spiral arms or significant dust lanes. The central bulge appears relatively bright, with a gradual decrease in luminosity towards the outer regions. The color profile suggests a dominant older stellar population, exhibiting a redder hue. There is no obvious evidence of recent or ongoing major mergers or tidal disturbances in the immediate vicinity, although the galaxy is slightly oblong rather than perfectly circular. The overall structure suggests a galaxy that has undergone significant evolutionary processes, potentially nearing a quiescent state in terms of star formation activity.