The galaxy appears as a relatively compact, elliptical structure. It exhibits a smooth light distribution, lacking prominent spiral arms or a distinct bulge. The overall color is somewhat reddish, suggesting an older stellar population with a lower rate of ongoing star formation. There is a slight asymmetry in the galaxy's shape, possibly indicating a minor interaction or disturbance, however the galaxy looks to be unperturbed. The galaxy displays an intermediate roundness and a significant population with round fractions. The morphology suggests a classification toward the early-type end of the Hubble sequence.
