The galaxy exhibits a morphology that appears to be a late-type spiral or possibly an irregular galaxy. There is evidence of a disk-like structure, although it may be somewhat disturbed or irregular. 

A central bulge is visible, displaying a yellowish hue. This suggests an older stellar population concentrated in the core. The disk presents a bluer color, particularly in localized regions, potentially indicating ongoing star formation. The galaxy does not appear to have well-defined spiral arms, and displays some patchy star formation, possibly indicating this is a merging galaxy.

The overall structure presents some irregularities, such as potential tidal features or asymmetric distribution of light, possibly due to a recent or ongoing interaction.
