The galaxy presents as a relatively smooth, centrally concentrated object, with a slight elongation, appearing more akin to a flattened spheroid than a spiral structure. Its overall color appears to be relatively even and consistent with an older stellar population. There is a slight indication of a possible minor disturbance present, though the galaxy is mainly intact. The main body of the galaxy displays a concentrated central region, but the outer regions are less defined with what may be a slightly dusty region. The appearance suggests a substantial fraction of the galaxy's light is emitted from a relatively compact, evolved stellar population, consistent with relatively low ongoing star formation.
