The galaxy presents as a luminous, ellipsoidal structure. The central region exhibits a high degree of concentration, with a smooth, seemingly featureless morphology. A noticeable elongation is present, suggesting a possible transition between an elliptical and lenticular classification. Fainter, diffuse emission extends from the central region, forming a more extended halo. There appears to be evidence of a minor disturbance, with a secondary condensation or tidal feature visible on one side of the galaxy's primary structure. The overall color of the galaxy appears relatively red, which suggests an older stellar population and lower levels of star formation.
