This galaxy exhibits a disk-like morphology, observed at a relatively high inclination. A central bulge component is apparent, displaying a yellowish-white color, suggestive of an older stellar population. The disk structure is evident through a flattened distribution of bluer light, likely indicating regions of active star formation. Faint redder hues appear towards the edges of the disk. There are hints of possible disturbances. Some asymmetrical features indicate it might be experiencing a minor merging event. Overall, the galaxy displays a mixture of old and young stellar populations distributed across its structure.
