The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical. It exhibits a yellowish-orange hue, suggesting a population of older stars. There is no apparent disk structure or spiral arm morphology visible, which further supports the classification as an elliptical galaxy. Faint signs of a possible minor disturbance or interaction can be seen in the outskirts of the galaxy. It appears relatively isolated, with no obvious signs of a recent major merger. The estimated physical size is about 6 kiloparsecs across. The absolute magnitude suggests it is a bright galaxy. It exhibits a low rate of star formation.
