The galaxy presents as a single, concentrated body with a smooth and generally featureless appearance. The central region exhibits a bright, somewhat diffused luminosity, transitioning to a fainter and more indistinct outer region. The shape appears close to circular, displaying minimal elongation or distortion. The color profile suggests a dominance of older stellar populations, leaning toward yellow and red wavelengths. There is no apparent evidence of spiral arms, dust lanes, or ongoing major merger activity. Faint disturbances are potentially present in the surrounding area, but these do not seem to dramatically effect the galaxy.
