The galaxy presents as a relatively smooth, elliptical-like structure, with a dominant central bulge. The light distribution appears concentrated towards the center, diminishing gradually towards the outer regions. There is some indication of a faint disk-like component, however this is not well defined. The overall color is yellowish, indicative of an older stellar population. There is a slight blueish tinge in the outer regions, which may indicate some ongoing star formation, but at a low rate. The galaxy does not appear to be heavily disturbed, although there is some irregularity in its shape, which might indicate a past or ongoing minor merger event.
