The galaxy presents as a relatively smooth, likely elliptical, structure. It appears to be largely featureless, exhibiting a gradual increase in luminosity toward its central region. Its ellipticity is moderate, exhibiting an intermediate form that is neither perfectly round nor highly elongated. There may be evidence of minor gravitational disturbance, indicating a possible past interaction or merger event. Coloration suggests a population of older stars, visible in the relatively redder hues compared to galaxies with ongoing star formation. The galaxy possesses a considerable mass and a low star formation rate.
