The galaxy exhibits a disk-like morphology, viewed at a slight angle from edge-on. There are hints of internal structure, with possible spiral arm features partially obscured by dust or lower surface brightness. A prominent central bulge is visible, appearing relatively smooth and concentrated. There is evidence of potential merging or tidal disturbances; there appears to be asymmetrical brightness.

The galaxy's color suggests ongoing star formation, with regions of bluer light indicative of younger stellar populations. Overall, the galaxy appears to be a disk galaxy undergoing morphological transformation.
