The galaxy presents as a spiral type. Two distinct spiral arms emanate from a moderately sized bulge. The arms exhibit a somewhat winding pattern, with a mix of medium and tight formations. The structure appears somewhat barred.

The central bulge exhibits a yellowish hue, indicative of an older stellar population. The spiral arms display a bluer tint, suggesting ongoing star formation. There is no visually obvious sign of major disturbances or recent merger activity, although some minor irregularities are apparent. The disk of the galaxy is close to face-on.
