The galaxy appears to be a spiral galaxy, presenting itself at a near edge-on orientation. While the disk is the prominent feature, it exhibits a degree of flocculence in its spiral arm structure. The spiral arms appear somewhat fragmented, with regions of active star formation discernible as slightly brighter, bluer knots within the disk. Dust lanes are subtly visible along the plane of the disk, creating a mottled appearance. There is an apparent central bulge that seems moderately bright and slightly elongated along the major axis of the disk. The bulge appears yellowish-white in color, suggesting a population of older stars. Overall, the galaxy exhibits characteristics of ongoing star formation within its disk and a relatively evolved bulge component. There may be some tidal disturbances or signs of interaction. The disk extends for what appears to be a significant distance, and seems to be moderately massive. The estimated size of the disk is approximately 7 kiloparsecs.
