The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It appears roughly circular in shape, displaying a moderate degree of roundness. A subtle color gradient is noticeable, with the core region exhibiting a slightly bluer hue compared to the outer regions, which appear redder. This color difference might suggest ongoing star formation in the central regions, with older stellar populations dominating the periphery. There is no clear evidence of spiral arm structure or a well-defined disk component. The overall light distribution is relatively even, with no major asymmetries or tidal features readily apparent. A hint of minor disturbance to the main body is possible, though indistinct. There is no strong evidence of a major ongoing merger event.
