The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a bright, concentrated central bulge region that dominates the overall luminosity. The bulge light seems to fade gradually into an extended halo with a slight flattening. The halo appears somewhat amorphous with hints of subtle structural features, but without distinct spiral arms or a well-defined disk. The overall color appears yellowish-red, suggesting an older stellar population with relatively little ongoing star formation. It appears to be fairly isolated, without obvious signs of interaction with nearby galaxies.
