The galaxy presents a clear spiral structure, observed at an oblique angle relative to our line of sight. Distinct spiral arms emanate from a bright, concentrated central bulge. The arms appear relatively tightly wound, displaying a flocculent morphology, and can be observed as having two or three major arms. Patches of blue coloration are visible within the spiral arms, suggestive of ongoing star formation activity. The central bulge exhibits a yellowish hue, potentially indicating a higher concentration of older stellar populations, while the arms show both blue and white hues, indicative of a mix of stellar ages. The galaxy does not appear to be undergoing any major merging events, though there may be minor tidal features present.
