This galaxy presents a prominent disk structure viewed at a shallow inclination. The disk exhibits spiral arm morphology, with two arms clearly identifiable. These arms display a moderate winding pattern, extending outwards from the central bulge.

The central bulge appears moderate in size and possesses a yellowish hue, suggestive of an older stellar population. The spiral arms show a bluer color, indicative of ongoing star formation. There is no strong bar-like feature detected, though the presence of a weak bar cannot be ruled out.

There are some minor disturbances, or distortions within the disk, which may be due to past minor merger events. Overall, the galaxy appears as a well-formed spiral structure.