The galaxy presents as a relatively smooth object with a concentrated central bulge. There appears to be a slight disk structure, but it lacks prominent spiral arms or distinct features. The galaxy is somewhat elliptical in shape. Color gradients suggest a possible variation in stellar populations, with the central regions appearing slightly redder than the outer disk. There is no strong evidence of a major ongoing merger or tidal disruption, though a minor disturbance cannot be ruled out. Overall, it resembles a lenticular or early-type spiral galaxy, potentially in the process of quenching star formation.
