The galaxy presents as a primarily smooth, elliptical-like structure. It exhibits a concentrated central bulge that emits a yellowish-white light, suggesting a population of older stars. Fainter, diffuse light extends outwards from the bulge, appearing almost spherical and diminishing in intensity. There may be subtle disk features present, but the galaxy is mostly a spheroid shape. There are no obvious signs of spiral arms or active star formation within the main body of the galaxy, although subtle disturbances could be present. The galaxy exhibits minimal signs of ongoing merger activity or significant tidal interactions. It appears relatively isolated in its environment.
