The galaxy presents a spiral morphology, exhibiting distinct spiral arm structures. The arms appear somewhat flocculent, with a moderate winding pattern. There is evidence of multiple spiral arms, potentially two dominant arms. The central bulge is noticeable but not exceptionally prominent, suggesting a possibly intermediate bulge size. The disk is viewed nearly face-on, obscuring any potential bar structure. There are some irregularities in the disk, possibly indicating minor disturbances, but overall the galaxy does not appear to be undergoing a major merger. The color gradient suggests a central concentration of older, redder stars, while the spiral arms exhibit bluer hues, indicative of ongoing star formation.
