The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated light profile, with the highest intensity towards the galactic center. The galaxy appears somewhat rounded in shape, with no discernible spiral arm structure. There is a slight disturbance observed within the galaxy, suggestive of a minor interaction, but there is no strong visual evidence of a major ongoing merger event. The overall color is yellowish/reddish, suggesting a population of older stars. The galaxy does not exhibit strong signs of active star formation, supporting the idea that it is composed of a population of aging stars. Based on its size and shape, the galaxy is most likely an elliptical galaxy with a low star formation rate.
