The galaxy presents as an elliptical morphology with a smooth, concentrated light profile. The core exhibits a bright, yellowish hue, indicative of a population of older stars. Moving outwards from the core, the galaxy appears to gradually fade, with a redder overall color. There is no clear evidence of spiral arm structure or significant dust lanes within the visible spectrum. Minor irregularities or disturbances are not readily apparent, suggesting a relatively undisturbed system. The shape appears close to round.
