The galaxy presents a smooth, somewhat elliptical morphology, with a highly concentrated central bulge. The light distribution decreases gradually from the bright nucleus outwards. There's a subtle, diffuse disk component surrounding the bulge, but it lacks distinct spiral arm structures. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or ongoing mergers, although there is some mild asymmetry present suggesting a past disturbance. The overall color is slightly redder in the bulge, and the blue component increases towards the edge of the disk suggesting the bluer color of young stars along the disk, though the colors are subtle. The object is relatively compact, with a moderate apparent size on the sky.
