The galaxy presents a generally elliptical morphology, appearing quite smooth with a high degree of central concentration. The light distribution is dominated by a central bulge, with a gradual falloff in intensity outwards. There is a subtle asymmetry present, though no obvious spiral structure or pronounced disk component is discernible in this imaging. There may be some evidence of minor tidal disturbance in the form of a slight asymmetry in the outer regions, but overall the galaxy appears to be relatively undisturbed. The galaxy is a reddish hue, indicating an older stellar population, typical of an elliptical galaxy.
