The galaxy presents as a spiral type, displaying a clear disk structure. Two prominent spiral arms emanate from the central region and appear loosely wound. The central bulge seems moderate in size, exhibiting a yellowish hue, which could be indicative of an older stellar population. There is a possible weak bar-like structure bisecting the bulge. Star formation appears to be occurring primarily in the spiral arms, as evidenced by their slightly bluer color compared to the bulge. The overall color indices suggest this galaxy is actively forming stars, although perhaps not at an extreme rate. There is no obvious sign of a major merger event, though some minor disturbances in the outer arms cannot be ruled out from this image alone. The disk is presented mostly face on.
