The galaxy presents as a spiral, viewed at an oblique angle. Its central bulge appears prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk is clearly visible, with a relatively high ellipticity. Faint spiral arm structures emanate from the bulge and fade into the outer regions. They are tightly wound. The overall color suggests that it is actively forming new stars, though at a moderately low rate. The galaxy does not exhibit strong signs of significant recent interactions or mergers, but the asymmetry in its outer regions might hint at minor disturbances. It has moderate amount of dust throughout.
