The galaxy presents as an elliptical or lenticular type, characterized by a dominant, smooth, spheroidal component. The central bulge appears bright and concentrated, exhibiting a yellowish hue indicative of an older stellar population. The overall light distribution is relatively even, lacking prominent spiral arm structures or distinct features. A faint, diffuse disk component may be present, subtly extending from the bulge. There's some slight suggestion of bluer, younger stars sparsely distributed in the outer regions. The galaxy doesn't show any obvious signs of ongoing major merger activity, although some minor distortions may indicate past interactions or minor disturbances. The shape is generally elliptical, with a slight elongation. 
