The object appears to be a spiral galaxy viewed nearly edge-on. A dust lane is visible bisecting the galaxy's bulge along its major axis, obscuring the starlight behind it. The bulge appears smooth and centrally concentrated, with a noticeable transition to a fainter and more extended disk. Faint spiral arm structures are weakly visible extending from the central bulge. There is likely little to no recent star formation activity, as evidenced by the redder color and lack of bright blue regions typically associated with young, massive stars. The galaxy does not display any significant signs of tidal distortion or interaction with neighboring galaxies. The estimated diameter is several thousand parsecs. The overall impression is of a relatively quiescent, disk-dominated galaxy.
