The galaxy presents a relatively smooth, elliptical morphology. It exhibits a yellow-orange hue, suggesting a population of older stars and relatively low ongoing star formation. The overall shape is somewhat elongated, displaying an axis ratio that deviates from a perfect circle. A slight, possible disturbance is visible on one edge of the galaxy, which may indicate a minor interaction with another galaxy or an internal dynamical process. There is no evidence of strong spiral arm structure or prominent dust lanes. The concentration of light is highest toward the center, gradually fading towards the outer regions. Overall, the galaxy appears to be a passively evolving system.
