The galaxy presents a generally elliptical morphology with a smooth light distribution. The galaxy is round in appearance. It exhibits a redder color profile in its central regions, which may indicate a higher concentration of older stellar populations. There is no visual evidence of spiral arms or significant dust lanes. The galaxy appears largely undisturbed. The object does not show any signs of tidal tails, strong gravitational lensing effects, or recent interactions with other galaxies. The integrated light suggests a relatively high stellar mass and moderate ongoing star formation.
