The galaxy presents as a somewhat elliptical structure. The central bulge appears bright and concentrated, exhibiting a yellowish hue indicative of an older stellar population. Fainter, bluer regions extend from the central bulge, suggesting the presence of younger stars and ongoing star formation. There is a subtle asymmetry, implying potential gravitational interaction or a recent minor merger event. Some slight disturbances in the outer disk of the galaxy may be evident. Overall, the galaxy appears to be in a transitional phase.
