The galaxy appears as a slightly elongated, disk-like structure. It exhibits a central bulge that is relatively prominent and appears more concentrated than the surrounding disk. The color gradient suggests a moderate level of star formation, with bluer hues visible within the disk possibly indicating regions of active star formation. The disk shows some irregularities but lacks the prominent spiral arm structures. Overall, this galaxy presents characteristics of a typical spiral galaxy without pronounced features such as strong spiral arms or a prominent bar. It also exhibits some degree of disturbance, though not so major as to significantly distort its morphology.
