The galaxy presents a somewhat amorphous structure, appearing neither purely elliptical nor a well-defined spiral. There's a central concentration of light, possibly indicative of a bulge component. The outer regions show some irregularities, hinting at possible tidal interactions or ongoing mergers. There appears to be some disk-like features. The galaxy exhibits a relatively red color profile, potentially suggesting an older stellar population and suppressed star formation. Faint blue hints in the disk may be indicative of some younger stars. Evidence shows that no major mergers have been observed, but the presence of disturbances cannot be ruled out. Overall, the galaxy's morphology suggests it's a galaxy undergoing some form of transformation or interaction.
