The galaxy presents as a relatively smooth, elliptical-like structure, with a dominant central bulge. The light distribution suggests a concentration of older stellar populations. The galaxy displays a subtle color gradient, shifting from a slightly bluer hue in the outer regions to a more pronounced reddish tint toward the core, indicative of differing stellar ages and compositions across the galactic body. There are indications of a possible minor disturbance. The galaxy is well-defined and is isolated.
