The galaxy presents as a lenticular or early-type spiral system, viewed at a near edge-on orientation. It exhibits a noticeable bulge component, with the light appearing concentrated and relatively smooth near the galactic center. The disk component appears diffuse and faint, extending horizontally across the image. The overall color profile indicates a system populated by older stellar populations, exhibiting a blueish-white hue. There is limited evidence of significant ongoing star formation. There may be minor disturbances in the disk, but the structure generally appears stable and unperturbed. The shape indicates that the galaxy appears to be relatively settled. The galaxy is compact in size.
