The galaxy presents as a centrally concentrated spheroid, likely an elliptical or S0 type. Its overall color appears to be a pale yellow-white, suggesting an older stellar population. The smooth light distribution indicates a lack of significant dust lanes or spiral arm structures. The galaxy displays a high degree of symmetry, and there is no visual evidence of ongoing major merging activity. There is potentially some asymmetry or minor disturbance in the galaxy's morphology, based on the faint extension on the left side of the galaxy. 
