The galaxy presents an elliptical morphology, with a smooth, concentrated central bulge. The light distribution suggests a relatively high Sersic index. The object exhibits a noticeable red color, indicating an older stellar population. The galaxy is observed at a redshift consistent with other spectroscopic measurements. There's a slight asymmetry in the outer regions which could be due to tidal interactions, although no obvious merger features are visible. The galaxy appears to be relatively isolated in its immediate vicinity, with a quiescent rate of star formation.
