The galaxy presents as a disk galaxy, oriented almost perfectly edge-on from our perspective. It exhibits a prominent central bulge, which appears slightly elongated. There is a noticeable change in color from the central bulge to the outer disk, with the bulge displaying a more yellowish or reddish hue compared to the somewhat whiter disk. The disk itself appears relatively smooth and lacks any obvious signs of distinct spiral arm structures or significant dust lane features. The overall morphology suggests a classification towards the later end of the Hubble sequence, though the lack of visible spiral arms makes it difficult to classify further. There is no evidence of any major ongoing merger events or significant tidal disturbances, though a very faint minor disturbance cannot be entirely ruled out.
