The galaxy presents as an edge-on spiral. A prominent, centrally located bulge dominates the visual morphology. The bulge exhibits a smooth texture and a rounded shape. The disk appears thin and elongated, oriented nearly parallel to the horizontal axis. The disk's color transitions from a bluer hue towards the outer edges, suggestive of more active star formation in those regions, to a yellower color near the bulge, which is indicative of an older stellar population in the center. There is no obvious distortion of the disk, and no signs of tidal tails, suggesting that this galaxy is not currently undergoing a major merger. Faint dust lanes can be tentatively identified along the disk plane, obscuring some of the starlight. There are some minor irregularities in the brightness of the disk, potentially indicating areas of enhanced star formation or density variations within the interstellar medium.
