The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. It has a bright, well-defined core that gradually fades into a diffuse halo. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct structural features within the main body. A subtle blueish color gradient is observed in the outer regions of the halo, possibly indicating some ongoing, albeit low, star formation activity. There is no evidence of significant tidal disturbances or interactions with other galaxies in its immediate vicinity. The overall appearance suggests a relatively evolved galaxy, likely an elliptical or lenticular type, with a substantial stellar mass.
