The galaxy presents a morphology consistent with a disk galaxy, observed at a moderate inclination. The central bulge appears significant, exhibiting a yellowish-orange hue, suggesting an older stellar population. A flattened disk extends outwards from the bulge, showing a mottled texture. The bluer colors observed throughout the disk suggest the presence of ongoing star formation. The disk does not appear perfectly smooth, showing subtle irregularities, possibly indicative of a minor interaction or recent accretion event, though major disturbances are not apparent. Overall, the galaxy appears relatively undisturbed, maintaining a well-defined structure.
