The galaxy presents as a single, centrally concentrated object with a smooth, elliptical morphology. The light distribution is centrally dominant, with a gradual decrease in surface brightness moving outwards from the core. The galaxy exhibits a yellow-orange hue, suggesting an older stellar population is dominant, with limited current star formation activity. The overall shape tends toward a slightly elongated spheroid rather than a perfect circle. There is a hint of a possible minor disturbance on one side of the galaxy, which could be the result of an ongoing or recent interaction or merger.
