The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. Its color profile exhibits a gradient transitioning from a yellow-white core to a redder outer halo. The galaxy is largely spheroidal, showing minimal evidence of a disk or spiral arms. No significant tidal features or signs of major mergers are apparent. There may be some low-level disturbance around the outer edges, however that is not clear. The light distribution suggests a relatively old stellar population dominating the galaxy's luminosity.
