The galaxy presents as a spiral type, exhibiting prominent spiral arm structures. These arms appear loosely wound. The galaxy's central bulge is moderately sized and exhibits a yellow-ish hue. The overall disk component appears to be larger than the bulge. The dust lanes within the spiral arms are moderately distinct. The galaxy's morphology is not significantly disturbed, indicating no recent major merging events. There is evidence of a bar structure. The galaxy is observed nearly face-on.
