The galaxy presents a generally smooth appearance with a high degree of central concentration. The object appears to be of elliptical morphology, or perhaps a spiral viewed nearly face-on with poorly defined spiral arms. It exhibits a moderate yellowish hue, suggesting a population of older stars. There is some evidence of interaction or merger activity in the form of a slight disturbance in its overall symmetry and faint surrounding features, although the main body of the galaxy remains largely undisturbed. The galaxy appears relatively compact, with an estimated size of around 6 kpc. Based on the color and smoothness of the galaxy, it likely exhibits a moderate amount of star formation, with an inferred stellar mass on the order of 10^11 solar masses.
