The galaxy presents as a somewhat face-on spiral or a lenticular galaxy, exhibiting a centrally concentrated bulge and a flattened disk structure. The galaxy displays a yellowish hue throughout the majority of its structure, indicative of an older stellar population. A disk is suggested by the slight edge-on view, though distinct spiral arms are not readily apparent. The overall form is fairly smooth and symmetrical. There is no sign of any tidal disturbances or close companion galaxies that might suggest recent or ongoing merger activity. Star formation appears moderate, with a relatively low rate of blue light, which is consistent with the yellowish appearance.
