The galaxy presents a moderately inclined spiral morphology. Two discernible spiral arms extend from a bright, concentrated central bulge. These arms exhibit a patchy structure, possibly indicating regions of active star formation. The overall color profile suggests a mix of stellar populations, with the bulge appearing yellower and the spiral arms showing bluer hues. There are subtle signs of possible gravitational interaction or minor disturbance in the outer regions of the galaxy. The galaxy possesses an approximate effective radius of 7.5 kpc. The inferred stellar mass is quite high, possibly on the order of 10^11 solar masses, with a relatively low star formation rate. A significant portion of citizen scientists classify the galaxy as smooth.
