The galaxy appears to be a spiral type, though the arms are somewhat ill-defined, presenting a more flocculent structure. The central bulge is prominent, with a yellowish-white hue, suggesting an older stellar population. The disk exhibits a bluer color, indicative of ongoing star formation. There is a slight asymmetry visible in the disk. The galaxy displays an overall smooth appearance with no major disturbances. A moderate amount of dust is visible within the disk structure. The shape of the galaxy is roughly circular.
