The galaxy presents as an edge-on spiral with a moderately bright central bulge. The disk appears relatively thin and elongated. There is a visible dust lane along the mid-plane, slightly obscuring the central bulge and adding to the apparent thinness of the disk. Faint blue star formation regions are observed within the disk, particularly noticeable along the outer edges, and likely traces the spiral arms. These regions indicate ongoing star formation. The overall color suggests a mixed stellar population with both older, redder stars concentrated in the bulge, and younger, bluer stars in the disk. There is no visible evidence of major mergers or tidal disturbances, though there appears to be a minor disturbance near the far right edge of the disk. The estimated size of the galaxy is several kiloparsecs across. The galaxy exhibits a high degree of edge-on orientation. The bulge displays a slightly rounded morphology.
