The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its central bulge is bright and concentrated, exhibiting a yellowish-white hue indicative of an older stellar population. The outer regions show a gradual decline in luminosity, fading into the background sky. There's a subtle color gradient visible, with the core appearing slightly warmer in color than the surrounding halo, which has a bluer tint. Overall, the galaxy appears to be well-formed with no obvious signs of major disturbances or ongoing mergers, though a minor interaction cannot be ruled out.
