The galaxy presents as an edge-on spiral, characterized by a relatively smooth and elongated disk. A central bulge is visible, though it appears subdued and somewhat rounded. There is a subtle color gradient along the major axis, with a slightly bluer hue apparent in the disk compared to the central regions. The disk exhibits little evidence of prominent spiral arm structure; however, there is a hint of dust lane obscuration along the mid-plane. Overall, the galaxy appears to be relatively quiescent, with low levels of star formation indicated by the lack of bright HII regions. It seems to be in a relatively isolated environment, as there are no obvious signs of tidal distortion or interaction with nearby galaxies. The outer regions of the disk fade gradually into the background sky, indicating a low surface brightness.
