The observed galaxy exhibits a disk-like morphology, viewed at a significant inclination angle. A central bulge component is present and appears yellowish, indicative of an older stellar population. The disk displays a mottled texture with regions of bluer hues, suggesting ongoing star formation. The galaxy is neither perfectly smooth nor significantly disturbed, with no clear signs of a major merger event. Some subtle asymmetries are present, potentially indicative of minor gravitational interactions. Overall, it is a relatively normal spiral or lenticular galaxy.
