The galaxy presents as an edge-on spiral, exhibiting a high degree of inclination relative to our line of sight. The central bulge appears prominent and exhibits a smoothly rounded morphology. A faint, extended disk is observed. The dust lane, indicative of a spiral galaxy, is observable and bisects the bulge. There are no signs of significant tidal disturbances. The galaxy appears relatively isolated. The core appears bright and its color suggests an older stellar population. There is a hint of blue color visible in the outer disk of the galaxy which suggest younger stars are found there. Based on the color and morphology, the galaxy's star formation rate seems suppressed.