The galaxy presents as a generally smooth, elliptical morphology. A concentrated central bulge appears distinctly orange, suggesting a population of older stars. The outer regions exhibit a gradual decline in luminosity. There is a subtle suggestion of a disk-like structure surrounding the bulge, oriented approximately horizontally in the image, however the arms do not appear very well defined, it appears to be a nascent disk. There may be minor evidence of a slight tidal disturbance or interaction, but it is not prominently displayed, but could be the reason the disk appears slightly disturbed. Based on its color and smooth texture, this galaxy is likely relatively massive with a stellar population that is not rapidly forming new stars.