The galaxy presents as an edge-on spiral with a prominent central bulge. The bulge exhibits a smooth, concentrated luminosity profile, appearing approximately spheroidal in shape. The disk component is thin and elongated, oriented nearly perpendicular to the line of sight. There is a possible slight warp or flaring evident in the outer regions of the disk, though higher resolution imaging would be necessary to confirm this. Color gradients suggest a redder, older stellar population dominates the bulge, transitioning to bluer, younger stars within the disk. No prominent dust lanes are discernible. There are no obvious signs of recent major merger activity or significant tidal disturbances. Faint light extends from the central bulge into the disk, which suggests the radius of the disk is approximately 7 kpc.
