This galaxy exhibits a moderately smooth morphology. It is primarily a diffuse object with a notable central bulge. The overall color appears to be slightly redder than the surrounding field, suggesting an older stellar population. There is faint evidence of a possible disk-like structure or tidal disturbance, but the signal is weak, perhaps due to the viewing angle or distance. There is a potential for minor interaction with another galaxy, as there may be some asymmetry in the outer regions of the object. It's difficult to tell, but it is possible that the object is a result of a galactic merger in progress. The lack of strong features indicates it is not undergoing active star formation. Further investigation and spectroscopic analysis would be required to confirm these observations.
