The galaxy appears as a luminous, elliptical structure. It presents a smooth, featureless profile, lacking prominent spiral arms or a distinct central bar. The core region exhibits the highest surface brightness, gradually decreasing towards the outer edges. The shape is observed to be somewhat elongated. Color gradients are subtle, with a slightly redder hue concentrated in the central bulge and a bluer tint becoming more prevalent in the outer regions. There is no apparent evidence of ongoing major merger activity or significant tidal disturbances. However, some minor asymmetry may be present in the extended halo.
