The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. A subtle disklike structure is not entirely absent, but the prominent feature is its rounded form. The central bulge is a yellow hue, indicating a population of older stars. Light tapers off from the center, but there is still a green hue that hints at some star formation occurring within the galaxy. There are no indications of ongoing major mergers or significant tidal disturbances, though there are some minor disturbances present. It has an estimated diameter of roughly 7 kpc. The color gradients observed across the galaxy suggest variations in stellar populations and star formation activity.
