The galaxy presents as a single, concentrated light source, roughly elliptical in shape. A bright, dominant core is observed, exhibiting a yellowish-white color. The intensity of light diminishes as the radial distance from the core increases. The outer regions display a more reddish hue and appear considerably fainter and more diffuse than the central core. No distinct spiral arms or disk features are readily apparent. The overall appearance suggests a relatively smooth light distribution. There is no evidence of significant ongoing star formation or dust lanes.
