The galaxy presents as a somewhat elliptical, disk-shaped structure, viewed at an oblique angle relative to our line of sight. There is a bright, concentrated central bulge region that appears almost spheroidal. Surrounding this bulge, a flattened disk component is visible. The disk appears relatively smooth, with little discernible spiral arm structure. The color distribution suggests varying stellar populations within the galaxy. The central bulge exhibits a whiter, potentially blue-shifted hue, possibly indicating the presence of younger, hotter stars or an active galactic nucleus. The outer disk exhibits a more reddish or possibly redshifted hue, potentially suggesting older stellar populations or dust obscuration. There appear to be some asymmetries and mild disturbances in the galaxy's morphology, potentially indicative of a past or ongoing interaction or merger event, though the primary structure is largely intact.
