The galaxy appears to be a spiral galaxy viewed at a moderate inclination. A prominent central bulge is observed, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component displays spiral arm structures, although they are not sharply defined and have a somewhat flocculent appearance. The arms display bluer regions indicating ongoing star formation within these regions. The galaxy does not appear to show any significant signs of a major merger. The morphology is fairly smooth and regular.
