The galaxy presents an overall smooth appearance, with a slightly elliptical shape. There is a noticeable concentration of light towards the center, suggesting a prominent galactic bulge. The colors are somewhat blended but a concentration of bluer light is seen toward one side of the galaxy, potentially indicating regions of active star formation. Conversely, a less prominent concentration of redder light exists on the opposing side of the galaxy. A subtle asymmetry and minor visible disturbances suggest the possibility of a past interaction or ongoing merger event. The galaxy is neither perfectly round nor highly elongated.
