The galaxy presents an elliptical morphology, elongated along a major axis. It exhibits a smooth luminosity profile, with the isophotes appearing generally well-behaved. The color is consistent with an older stellar population, showing a redder overall hue, though some internal color gradients could be present. There is no definitive presence of a disk, spiral arms, or a prominent central bar. It displays some slight indications of tidal disturbance. The red shift indicates that this is a distant galaxy. It seems to be a relatively massive system with some star forming activity, although at a low rate. Overall, the galaxy appears as a relaxed system, likely an evolved galaxy transitioning towards a passive state.
