The galaxy appears to be a spiral galaxy, seen at an oblique angle. It exhibits a bright, concentrated central bulge that appears yellowish-white in color, suggesting an older stellar population. The disk surrounding the bulge shows a mottled texture, hinting at the presence of spiral arms. The arms are not well-defined, exhibiting a flocculent structure with regions of blueish light intermixed with what appear to be dust lanes. The blueish regions suggest areas of active star formation. The galaxy does not appear to be strongly interacting or merging with any other galaxies, but there may be some minor disturbances in the disk or outer halo.
