The galaxy presents a largely smooth morphology, exhibiting a centrally concentrated bulge with an elliptical shape. The light profile appears relatively uniform, lacking distinct spiral arm structures. There is some evidence of faint, diffuse features, though they are not sharply defined. The colour appears to be generally redder and consistent with an older stellar population with a relatively low rate of star formation. There are no clear indications of tidal disturbances or ongoing mergers.
