The galaxy presents as a spiral type, though the spiral arms are not sharply defined. It exhibits a prominent central bulge that appears nearly spherical and is considerably brighter than the surrounding disk. The disk component shows a mottled texture, possibly indicating regions of active star formation, although dust lanes are not clearly visible in this image. The galaxy is viewed at an oblique angle, not quite edge-on but showing a noticeable flattening. There appears to be a weak bar structure extending through the bulge region. Overall, the galaxy shows characteristics of intermediate mass, with moderate star formation activity. There does not appear to be any major merger activity.
