This galaxy exhibits a clear disk morphology and is seen nearly edge-on. The central bulge appears bright and somewhat rounded, with a yellowish hue suggesting an older stellar population. A distinct dust lane bisects the galaxy, obscuring light from stars in the disk and the near side of the bulge. Star formation appears concentrated in the plane of the disk, inferred by the slightly bluer color along the edges of the disk, but has no particularly remarkable features. The lack of obvious tidal features suggests the galaxy is relatively isolated and quiescent, with a morphology consistent with a spiral galaxy experiencing relatively low levels of star formation. There are no indications of significant interaction with other galaxies, however, there seems to be a slight warp in the plane of the disc, hinting at a possible minor interaction in the distant past.
