The galaxy presents a generally elliptical morphology, appearing largely smooth and relatively undisturbed. Its light profile shows a central concentration of brightness that gradually fades towards the outer regions. The main body of the galaxy appears almost round, with only a slight elongation, and a generally uniform color, suggesting a population of older stars. There is no apparent dust lane or any clear spiral structure. It has a compact appearance, indicating that star formation may be low, but there is a bluer tinge implying some star formation may be occurring.
