The galaxy appears to be an elliptical galaxy, presenting a smooth and somewhat spherical morphology. There is no visible disk structure or spiral arms discernible. The central region exhibits a high degree of concentration, indicated by the bright and compact core that dominates the galaxy's light distribution. The galaxy appears to be relatively isolated, with no major disturbances. The colour appears to be leaning toward red, suggesting an older stellar population and potentially lower star formation activity. 
