The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. A central bulge is apparent, exhibiting a smooth, rounded morphology. Dust lanes are subtly visible, extending along the equatorial plane of the galaxy, particularly obscuring the bulge region. The disk appears relatively smooth, with a faint, diffuse luminosity gradient extending outwards from the central bulge. The galaxy displays a gradient of color across its structure. The central bulge appears to be composed of older stars and is likely a brighter shade of yellow, while the outer disk appears to be more bluish, indicating the presence of younger, hotter stellar populations. No spiral arm structure is clearly discernible. There is no evidence of a major merger or strong tidal disturbances.
