The galaxy presents as a face-on spiral, exhibiting a moderate degree of central bulge prominence. Spiral arm structures are visible, although somewhat flocculent and not sharply defined. A hint of blue is visible in these arms, suggestive of ongoing star formation. The central region appears more yellow-white, indicating an older stellar population. The galaxy shows a slight ellipticity, with the major axis oriented approximately northeast to southwest. The disk is not perfectly smooth; some irregularities are present. There does not appear to be any ongoing major merger event, but a possible minor disturbance in the outer regions of the disk warrants further investigation.
