The galaxy appears to be a spiral galaxy, though its disk is somewhat faint. There is a central bulge region that appears more luminous and relatively smooth. Faint spiral arms emerge from the bulge. The galaxy is not observed perfectly face-on; instead, it is at a slight angle to our line of sight. The color distribution suggests active star formation, with bluer regions visible in the spiral arms. There is no apparent disturbance or major merger events occurring within the galaxy, although one arm is slightly disrupted. The galaxy is not barred.