The galaxy presents as a centrally concentrated, roughly circular object. The light distribution appears smooth, with no discernible spiral arms or distinct substructures visible. The central region is significantly brighter than the outer regions, suggesting a prominent bulge or nucleus. The color profile indicates a general yellowish-red hue, which may indicate an older stellar population and a relatively low rate of ongoing star formation. There are no obvious signs of tidal disturbances or interactions with other galaxies. The overall morphology suggests an elliptical or lenticular galaxy type.
