The galaxy presents as a spiral type, with a noticeable disk and a prominent central bulge. The spiral arms are distinct, displaying a loosely wound morphology, and appear bifurcated, with two dominant arms visible. There is a faint indication of ongoing star formation activity within the arms, evidenced by the slightly bluer hues in those regions compared to the bulge. The central bulge exhibits a yellowish-orange color, suggesting an older stellar population. Overall, the galaxy's disk exhibits a smooth appearance, although some minor irregularities and disturbed features are present, indicating a potential recent or ongoing interaction with a smaller galaxy or tidal effects. The galaxy is not seen perfectly face-on, but rather at a slight angle. No significant bar structure is discernible.
