The galaxy presents as a barred spiral, viewed at an oblique angle, exhibiting an overall bluish hue indicative of ongoing star formation. Two distinct spiral arms emanate from a central, somewhat elongated bar structure. These arms appear moderately tightly wound. A bright, compact central bulge is evident, though not dominant in size compared to the overall disk. There are no indications of any major merging events occurring with the galaxy, but there are some minor disturbances of disk symmetry. The galaxy appears to be moderately elliptical, and its structure is composed of a prominent disk and a moderate central bulge.
