This galaxy exhibits a disk-like structure, observed at an inclined angle. The disk presents a mottled appearance, with evidence of spiral arm fragments visible as slightly brighter, bluer regions against a more diffuse background. These regions suggest ongoing star formation. A central bulge is apparent, appearing smoother and brighter than the disk component. There are no indications of a strong bar feature or a clear spiral pattern from what can be seen in the image. Overall, the galaxy appears to be undergoing some level of star formation activity within its disk, with a relatively smooth, and moderately prominent bulge. There is evidence of possible minor tidal disturbance.
