The galaxy appears as a single, relatively smooth object. It displays a near-perfect elliptical morphology, with no discernible spiral arms or bar structures. The light distribution suggests a high degree of central concentration, with luminosity decreasing smoothly from the core outwards. There is a suggestion of a slight elongation, but the galaxy is largely round. The galaxy has an overall yellowish-orange hue, indicating a likely dominance of older stellar populations. There are no obvious signs of recent major merger events or strong tidal interactions with neighboring galaxies. The outer regions appear diffuse, gradually blending into the background sky, without any sharp edges or prominent features.
