The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be somewhat spheroidal in shape, with a bright central bulge. There is a subtle color gradient, with the core exhibiting a yellowish-white hue, suggestive of an older stellar population. The outer regions show hints of a bluish tint, potentially indicating the presence of younger, hotter stars, although this is not very prominent. There's little evidence of defined spiral arms or a prominent disk. The overall appearance suggests that it is a galaxy with low ongoing star formation. There are hints of minor disturbances in the morphology, but no large scale interactions or mergers are apparent.
