The galaxy presents a largely smooth, elliptical morphology, with little evidence of spiral arm structure.  The overall color profile suggests a relatively old stellar population, appearing yellow and redder in the optical bands, indicative of lower star formation. The concentration of light towards the center is significant, indicating a dense core, but there is not an indication of a highly active galactic nucleus. The galaxy appears fairly isolated; there is no obvious sign of tidal interactions, such as streams or distortions, which suggests it is not currently undergoing a major merger. The lack of substantial blue light implies that the galaxy has a suppressed star formation rate and the overall morphology is consistent with a relatively high-mass system.
