The galaxy appears to be a relatively smooth, elliptical galaxy. Its light profile suggests it is highly concentrated. There is a noticeable absence of distinct spiral arms or prominent dust lanes. The overall color seems to be consistent with an older stellar population, indicating that the galaxy's star formation rate is relatively low. The isophotes appear mostly round, deviating minimally from a perfect circle. There is no evidence of any major ongoing mergers or tidal disturbances, though there appears to be some minor irregularity in the outer regions.
