The galaxy presents as a relatively faint, edge-on spiral, exhibiting a high degree of inclination relative to our line of sight. A prominent central bulge dominates the galaxy's morphology, appearing smoothly textured with a yellowish hue, indicative of an older stellar population. The disk is elongated and appears relatively thin. There appears to be an absence of substantial dust lanes visible along the disk, although some obscuration may be present, subtly affecting color and brightness. There may be some minor irregularities present in the disk, hinting at a possible recent or ongoing minor interaction, but this is difficult to confirm. The overall structure appears relatively undisturbed.
