The galaxy presents as a relatively smooth, elliptical-like structure. It appears moderately bright with a somewhat diffuse profile, suggesting a substantial stellar population. There may be a faint, very slightly bluer center, possibly indicating the presence of younger stars or an active galactic nucleus, though this is difficult to confirm given the image resolution. The overall color is suggestive of a galaxy dominated by older stellar populations, likely with low current star formation activity. There is some evidence of minor disturbances in its shape, which hints to a possible past merger event, though the primary structure remains largely undisturbed. The galaxy's apparent roundness suggests it is closer to face-on with respect to our line of sight.
