The galaxy appears to be a spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, concentrated structure with a yellowish-orange hue, suggestive of an older stellar population. Fainter, bluish spiral arms extend outwards from the bulge, indicating regions of active star formation. The arms are not well-defined, appearing somewhat patchy and flocculent. The disk of the galaxy shows moderate inclination. There is subtle evidence of tidal features or minor disturbances in the outer regions of the galaxy, but no signs of a major merger. The galaxy is overall characterized by intermediate star formation.
