The galaxy presents a generally smooth morphology. The light distribution appears relatively uniform, lacking prominent spiral arms or a well-defined bar structure. It exhibits a concentrated central bulge transitioning into a more diffuse halo. 

The color profile appears to be redder in the core with bluer halos, indicative of an older stellar population concentrated in the nucleus, surrounded by a population of younger stars. 

The shape is approximately elliptical. There is no obvious evidence of significant tidal disturbances or ongoing mergers, although minor asymmetries or faint extensions could potentially be present upon closer inspection. The system overall exhibits characteristics of a relatively massive galaxy, likely an elliptical or lenticular type galaxy.
