The galaxy presents as a disk galaxy, observed nearly edge-on from our vantage point. The nucleus appears as a bright, concentrated bulge, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component is subtly visible, extending outwards from the bulge with a relatively smooth texture and less intense coloration, displaying a slightly reddish tint. There is a possible asymmetry in the disk, which may suggest a slight warp in the disk or a possible ongoing minor merger. The overall morphology appears relatively undisturbed with no major disturbances or clear signs of interaction from the visual inspection of the galaxy. No prominent dust lanes are discernible. The galaxy does not exhibit features indicative of significant star formation, lending to the older stellar population suggested by color.
