The galaxy presents as a relatively bright, face-on spiral with well-defined spiral arms. The arms exhibit a somewhat flocculent structure, displaying a patchy distribution of star-forming regions. A central bulge is discernible, appearing moderately sized and yellowish in color, suggesting a population of older stars. The disk component is noticeably bluer in contrast, indicating ongoing star formation. There is no evidence of a strong central bar feature, but a weak one is potentially present. While the galaxy appears largely undisturbed, there may be minor distortions, possibly hinting at a past or ongoing interaction or merger event. The galaxy is not edge-on, the features of the disk are clearly visible.
