The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light distribution appears centrally bright, decreasing gradually towards the outer regions. The ellipticity is moderate, suggesting a classification somewhere between E3 and E5 on the Hubble scale. The color gradient indicates a redder core transitioning to slightly bluer outskirts, which implies older stellar populations are more centrally located, with possibly some recent or ongoing star formation in the outer regions. Evident is a small, amorphous disk. There is no indication of strong tidal features or ongoing major mergers. The galaxy appears relatively undisturbed, showing only minor signs of morphological disturbance in the form of fuzziness in the outer regions.
