The galaxy exhibits a primarily smooth morphology, suggesting an elliptical or lenticular classification. It presents with a relatively rounded appearance. There is a noticeable color gradient, transitioning from bluer hues near the center to redder tones in the outer regions. This could indicate differing stellar populations or dust distribution.

Based on visual inspection, there does not appear to be a dominant spiral structure or prominent disk feature. However, the presence of some degree of irregularity or minor disturbance cannot be entirely ruled out. There may be some evidence of a merger event, or other gravitational interaction. The color profile of the galaxy suggests it is mature, and has likely consumed a significant amount of its gas. 
