The galaxy presents as a somewhat amorphous, moderately luminous object. The central region exhibits a bright, concentrated core, suggesting a higher density of stars and possibly a supermassive black hole actively accreting matter. The galaxy's overall color appears slightly blue-shifted, indicating active star formation. The galaxy's morphology is largely smooth with a slight disk shape, though subtle irregularities are visible, suggesting a possible interaction or recent merger event. Evidence for this can be seen in the slight disturbances to the shape of the galaxy. Further observations would be required to verify the precise nature of the observed disturbances.
