The galaxy presents as a moderately bright, elliptical form. It displays a centrally concentrated bulge that fades gradually into a less defined halo.  The overall color is a soft blue-white, suggestive of a population of relatively young, hot stars. While the overall structure is relatively smooth, there is a subtle hint of a disk-like structure, though not clearly defined.  No strong signs of recent or ongoing major mergers are visible, although some subtle irregularities indicate minor gravitational interactions might be occurring. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. The galaxy has a low rate of star formation.
