The galaxy presents a clearly defined disk structure, viewed at an angle that reveals a flattened, somewhat elliptical shape. Observable spiral arms are present. The central bulge appears relatively small and dim. The disk shows some irregularities, with some brighter regions suggesting areas of active star formation, with noticeable variations in color. The galaxy does not appear to be undergoing a major merger, but subtle disturbances could indicate recent or ongoing minor interactions. The galaxy overall exhibits a blue hue, indicative of ongoing star formation activity. The outer edges of the disk fade gradually, and the dust lane distribution may hint at internal structures, with some patches or dark regions potentially obscuring light from behind. There is no obvious bar structure within the central bulge.
