The galaxy presents as a slightly inclined spiral galaxy with a prominent bulge. The bulge appears to be smooth and centrally concentrated, with a yellowish hue. The disk is visible, showing a faint hint of spiral arm structure. The arms are not sharply defined, appearing somewhat flocculent and patchy. The disk appears bluer than the bulge, possibly indicating regions of ongoing star formation. The galaxy appears to be relatively isolated. The galaxy exhibits a moderate level of ellipticity.
