This galaxy exhibits a prominent spiral structure with two well-defined arms. The arms are loosely wound, extending outward from a central bulge. The bulge is relatively compact and appears yellowish, indicative of an older stellar population. The spiral arms display a bluer hue, suggesting the presence of ongoing star formation. There are no signs of major merger activity, although there is a slight asymmetry observed in one of the arms, indicating a possible minor disturbance or interaction. A weak bar feature may be present across the central bulge, but it is not a dominant characteristic. The galaxy is not edge-on, as the disk is clearly visible.
