The galaxy presents as a relatively compact object with a somewhat diffuse morphology. It appears to have a generally spheroidal shape but with some notable irregularities and extensions suggesting potential tidal features. The light distribution is concentrated in the central region with a smoother component extending outwards.

Color gradients are present, with a generally redder hue in the central regions and a bluer coloration in the extended features. These color variations could indicate varying stellar populations or dust content within the galaxy. There also appears to be some disturbance in the form of clumpy regions or possible remnants of an interaction. These structures suggest that the galaxy may have undergone a minor merger.
