The galaxy appears as a roughly elliptical, disk-shaped object with a bright central bulge. The core is intensely luminous, exhibiting a cyan hue, suggesting possible active galactic nucleus activity or a high concentration of young, hot stars. Fainter light extends outwards, and a slight distortion on one side might indicate a minor gravitational interaction or disturbance. Overall, it appears to be a relatively compact galaxy. There is no obvious spiral structure or prominent dust lanes. The light distribution seems relatively uniform, with a gradient decreasing from the bright center outwards.
