This galaxy exhibits a morphology consistent with a spiral galaxy. The central region presents a prominent bulge, exhibiting a yellowish hue, which indicates the presence of an older stellar population. Extending outwards from the bulge are two well-defined spiral arms, wound moderately tightly around the galactic center. These arms appear bluish, suggesting regions of ongoing star formation. There is no evidence of significant tidal disturbances or ongoing major mergers within the galaxy's morphology. Subtle asymmetries might indicate minor gravitational interactions. There is a suggestion of a bar-like structure bisecting the central bulge region, though this is not definitively confirmed. The galaxy displays a clear disk component viewed at a near-face-on angle. Overall, it appears to be a well-formed spiral galaxy with active star formation regions in its arms.
