The galaxy presents a morphology that is largely smooth and elliptical in appearance, with some features suggesting possible disturbances. The central bulge is a dominant feature, exhibiting a bright yellowish-orange hue, indicating a population of older stars. There is a faint disk component which appears relatively thin.

Evidence of a possible minor disturbance is visible in the form of a slight asymmetry and an arm-like extension that may indicate interactions or past merger events. Patches of redder regions may indicate star forming regions. It has a moderate to high mass and a low but non-zero star formation rate.
