This galaxy appears to be a spiral galaxy, viewed at a slight angle but not quite edge-on. Prominent spiral arms are visible, exhibiting a somewhat flocculent structure. The central bulge is relatively large and appears to be moderate in size, dominating the inner region of the galaxy. A bar structure is either not present or is very weak. The galaxy exhibits a moderate amount of star formation, indicated by the slightly bluer color in some of the spiral arms. No major merging events or significant tidal disturbances are apparent, though the galaxy is likely undergoing minor interactions. The overall color gradient suggests a higher concentration of older stellar populations towards the bulge, with younger, bluer stars populating the spiral arms.
