This galaxy presents as a disk-shaped system oriented edge-on relative to our line of sight. A prominent central bulge is observed, exhibiting a yellowish-white hue, suggestive of an older stellar population. The disk component appears relatively smooth, lacking readily discernible spiral arm structures or prominent dust lanes. There is a subtle color gradient moving from the central bulge outwards through the disk. The outer regions of the galaxy are less luminous. The overall structure indicates a mature galaxy that does not appear to be undergoing major merger activity.
