The galaxy presents as a roughly elliptical structure, exhibiting a smooth, diffuse morphology. The central region shows a distinct concentration of light, indicating a possible bulge. A color gradient is observable; the core appears reddish, possibly indicative of an older stellar population, while the outer regions display a bluer hue, which could signal younger stars and ongoing star formation, albeit at a moderate rate. There is a subtle suggestion of possible minor disturbances in the outer structure, but further examination at higher resolution would be needed to confirm this. There is no evidence of a major merger event, however, smaller interactions cannot be ruled out.
