This galaxy appears to be a spiral galaxy with a prominent central bulge. The bulge appears moderately sized relative to the disk. The disk component shows evidence of spiral arms, which are somewhat tightly wound and not particularly well-defined, appearing more flocculent in nature. There are no signs of a prominent bar feature. The galaxy exhibits a blue hue, suggesting the presence of ongoing star formation, particularly within the spiral arms. There is no evidence of major mergers or significant tidal disturbances. The overall morphology suggests a relatively undisturbed spiral galaxy undergoing moderate star formation.
