This galaxy appears to be an elliptical galaxy, characterized by a smooth, diffuse morphology. It exhibits a centrally concentrated luminosity profile with a gradual decrease in brightness outward. The overall color of the galaxy appears relatively uniform, with a slight suggestion of a redder hue in the outer regions compared to the core. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy displays a high degree of roundness and a lack of significant tidal features or distortions, suggesting it is likely a relatively relaxed system that is not currently undergoing a major merger event. However, there may be some minor disturbances visible in the image. Judging from the color, the galaxy contains a population of older stars and exhibits a low star formation rate.
