The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal with a high degree of central concentration. The light distribution is quite uniform, with no obvious spiral arm structures or significant dust lanes.

The galaxy core exhibits a bright, concentrated luminosity. Colors appear somewhat redder, possibly indicating a population of older stars, with little to no ongoing active star formation occurring in the central bulge. The galaxy's outer regions show a gradual decrease in light intensity. These outer regions are still quite smooth, but there may be a hint of a very faint disk component. There is no clear evidence of a merger, or major tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed system.
