The galaxy appears as a largely featureless elliptical, exhibiting a smooth and diffuse luminosity profile. It displays an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. The core of the galaxy is brighter, suggesting a concentration of older stellar populations. Faint reddish hues are seen in the central regions and may indicate older stars. There are no significant indications of strong star formation regions or spiral arm structures. The galaxy is undisturbed, without evidence of recent major mergers or tidal interactions. Minor disturbances may be present.
