This galaxy presents as a spiral, viewed at a considerable angle but not quite edge-on. A defined central bulge is visible, appearing roughly spherical and concentrated. Evidence of disk structure is observable, but not fully resolved, with some areas showing enhanced luminosity that suggest higher concentrations of star formation, tracing the spiral arms. The disk appears to be undergoing a significant merging event with another galaxy. This may be inducing an elevated star formation rate within the spiral disk as the result of tidal disturbances from the merging galaxy. The overall color profile indicates a mix of stellar populations, with bluer hues in the outer regions suggesting recent star formation and redder tones in the central bulge hinting at an older stellar population. The galaxy's morphology is irregular, likely influenced by the ongoing interaction.
