The galaxy presents as a moderately inclined spiral galaxy, exhibiting a disk-like morphology. The central bulge appears relatively prominent and concentrated, displaying a yellowish hue, suggestive of an older stellar population. The spiral arms are somewhat flocculent and exhibit a bluer color, hinting at ongoing star formation. The arms appear somewhat tightly wound. There appears to be some dust lanes within the disk and along the spiral arms, which is obscuring some of the light. Overall, the galaxy appears relatively isolated, and its structure is reasonably undisturbed, showing no obvious signs of major mergers, although some minor disturbances in morphology cannot be ruled out. The galaxy's light is concentrated within a defined area, and it shows a smooth overall profile.
