The galaxy appears to be an elliptical morphology, with a smooth, centrally concentrated light distribution. The overall color of the galaxy is yellowish-white, suggesting a population of older stars. There is little evidence of spiral arms or prominent dust lanes. The isophotes appear relatively smooth, suggesting a relaxed dynamical state. The ratio of the semi-minor to semi-major axis is approximately 0.8, indicating a moderate degree of ellipticity. The outer regions of the galaxy fade gradually, and the radius containing 50% of the light is a little less than half of that containing 90% of the light, which demonstrates a high concentration of light towards the center. There is no clear sign of a galactic nucleus.
