The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, appearing nearly circular in projection, with a gradual decrease in luminosity moving outwards. The core region is the brightest, displaying a yellow-white hue. There is a subtle color gradient, with the outermost regions appearing slightly redder compared to the core. No distinct spiral arms or significant dust lanes are readily apparent. The overall appearance suggests a relatively evolved stellar population, consistent with a passively evolving system. There is no evidence of any major disturbances to the main body of the galaxy.
