This galaxy exhibits a distinct spiral structure. The spiral arms appear well-defined, showing a relatively tight winding pattern. The galaxy possesses a prominent central bulge, although its size appears moderate in relation to the overall disk. Indications suggest a possible bar structure is present across the center, but it is hard to say for sure from the image.

There are disturbances present in the disk, hinting at a possible merger with another galaxy, or some sort of gravitational interaction. This is supported by the tidal tail extending from the main body of the galaxy. Despite this, there are large portions of the galaxy that are not noticeably affected by the disturbance. The color indices also indicates there is active star formation present in the disk. 
