The observed galaxy presents as a barred spiral galaxy, inclined significantly to our line of sight. A central bulge exhibits a smooth, concentrated luminosity profile with a yellowish-red color, likely indicating an older stellar population. The disk of the galaxy shows evidence of spiral arm structure, although the arms are somewhat flocculent and lack high definition. The arms display a bluer color, indicative of ongoing star formation.  Dust lanes are visible along the inner edges of the spiral arms. The overall shape is elliptical, due to the viewing angle. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interaction or significant morphological disturbance.
