The galaxy presents as a lenticular or edge-on spiral system, appearing as an elongated, flattened structure. A central bulge is visible, exhibiting a relatively smooth and concentrated light distribution. A faint disk is observed, subtly extending from the bulge, with a slight bluer hue. There is no strong evidence of distinct spiral arms. There may be a slight warp to the disk. There are no obvious signs of any active mergers or major disturbances in the galaxy's morphology, though minor disturbances cannot be ruled out. The colors appear slightly bluer in the disk, which is consistent with some ongoing star formation, although at a low rate. Overall, the galaxy exhibits a fairly regular and relaxed morphology.
