The galaxy appears to be elliptical in shape, with a high degree of smoothness. Its light distribution is concentrated towards the center, suggesting a relatively old stellar population. There is a subtle color gradient, with the core appearing slightly yellower than the outer regions, possibly indicating a higher concentration of older, redder stars in the nucleus. Some potential signs of a minor disturbance can be seen in the arm with some dust and gas clumps that have some regions of light and color variations. Overall, the galaxy presents as a relatively undisturbed and evolved system.
