This galaxy presents as an elliptical-like morphology, appearing largely smooth and spheroidal in shape, with no discernible spiral arms or a prominent central bar. Its light profile appears relatively uniform, with a gradual decrease in brightness from the core outwards. There is some evidence of possible minor disturbances in the outer regions of the galaxy, such as faint asymmetric features, but no significant merger activity is clearly indicated in the image. The overall color of the galaxy appears slightly redder than the average background stars, suggesting a moderate presence of older stellar populations and/or dust content. Its estimated size is substantial, indicating that it is likely a massive galaxy.
