The galaxy presents as a spiral type, inclined with respect to our line of sight. There appears to be a prominent central bulge, extending along the major axis. The bulge has a moderate size compared to the rest of the disk. Faint spiral arms are visible, though not sharply defined. The bluer color in certain regions, especially the center and upper part of the disk suggests ongoing star formation. There appears to be a bar feature traversing the bulge. The disk exhibits some irregularity, potentially indicative of minor gravitational interactions or disturbances. No major merger events appear to be occurring at present. The overall color suggests a mature stellar population, with younger, bluer stars contributing to the star-forming regions.
