The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears generally round, with only a slight deviation from perfect circularity. There are no obvious spiral arm structures or prominent dust lanes visible. The color of the galaxy is predominately yellowish-orange, suggesting an older stellar population with a relatively low rate of ongoing star formation. The lack of blue light indicates a scarcity of young, hot, massive stars. The galaxy exhibits some signs of tidal disturbance, possibly indicative of a past or ongoing merger event. The outer regions appear somewhat fuzzy, without a well-defined edge, which could be caused by interactions with another galaxy.
