The galaxy presents as a spiral with a clearly defined disk structure. The spiral arms are prominent and moderately wound. The color suggests active star formation is present, particularly within the arms where a bluer hue is evident. The central bulge is moderately sized and appears relatively bright, possibly indicating an older stellar population. There is no evidence of a strong bar feature bisecting the bulge, though a weaker bar cannot be ruled out. There appear to be two well-defined spiral arms with distinct pitch angles. The overall structure suggests that this galaxy has not recently undergone a major merger event, though minor gravitational disturbances may be present.
