This galaxy presents as an edge-on spiral system, characterized by a prominent, elongated disk structure. The central bulge appears significant, exhibiting a relatively smooth and rounded morphology. A dust lane is not clearly discernible, obscuring the light from stars in certain regions. There appears to be modest star formation, with some evidence of ongoing activity within the disk region. The system displays no obvious signs of major tidal disturbances or ongoing mergers with other galaxies, suggesting that it has remained relatively isolated during its evolutionary history. Based on its color profile, with an overall red appearance with some bluer regions, the galaxy may have a population of intermediate-age stars.
