The galaxy presents as a spiral with discernible arms. These arms exhibit a clumpy morphology, hinting at regions of active star formation. A central bulge is visible, though it appears to be relatively small compared to the overall disk size. The disk itself seems prominent, with a relatively low inclination to our line of sight. There is no evidence of a strong central bar structure within the galaxy's disk. No major signs of ongoing or recent major merger events are apparent. The galaxy appears relatively undisturbed in its morphology. There is a color gradient across the galaxy, with the central regions exhibiting a slightly redder hue, potentially indicative of an older stellar population or higher dust content, and bluer outer arms that would be indicative of a younger stellar population. The galaxy's size is moderately extended on the sky, and a smooth component may be present throughout the object.
