The galaxy presents as a relatively smooth, elliptical or lenticular system. There is a concentration of luminosity towards the central region of the galaxy, suggesting a prominent bulge. The outer regions appear fainter and less defined, with a gradual decline in surface brightness. No distinct spiral arm structures or dust lanes are discernible. The color appears overall to be somewhat redder and more yellow throughout with some blue in the outer regions, indicative of an older stellar population. It exhibits an approximate average roundness. There is no strong evidence of ongoing major mergers or tidal disturbances within the system.
