The galaxy presents a largely smooth, elliptical morphology, exhibiting a concentrated central bulge that appears yellowish-orange, indicative of an older stellar population. There is a slight extension of the galaxy on the left side, and the shape has a moderate degree of roundness. The faintness of any visible disk features suggests a relatively low star formation rate. The overall appearance suggests the galaxy is not currently undergoing any major merging events, though some minor disturbances cannot be ruled out. The angular size is relatively small, indicating a significant distance.
