This galaxy presents as a largely spheroidal object, exhibiting a smooth, diffuse profile with a highly concentrated central bulge. The core region displays a distinct yellowish-orange hue, likely indicative of an older stellar population. Moving outward from the center, there appears to be a gradual transition to fainter, less defined regions, with subtle color variations possibly suggesting ongoing or recent star formation. Overall, the galaxy's morphology suggests an elliptical or lenticular classification, with a moderate amount of internal activity based on the color gradients. There are subtle hints of asymmetry or minor disturbances in the outer regions, potentially pointing to past interactions or mergers, though the dominant impression is that of a relatively undisturbed, evolved system.
