The galaxy presents an elliptical morphology with a smooth, largely featureless appearance. The galaxy exhibits a concentrated central bulge that is yellowish in color, indicating an older stellar population. The outer regions are less defined, with a gradual decrease in luminosity. There is no apparent spiral arm structure or significant dust lane obscuration. The overall shape appears to be slightly elongated but generally round. There is no evidence of any major ongoing merger activity or significant tidal disturbances. The galaxy appears to be relatively isolated.
