The galaxy presents a somewhat elliptical morphology, exhibiting characteristics of both smooth and featured structures. The central region appears as a bright, concentrated bulge, possibly indicative of a high density of stars. A faint, extended disk is discernible, suggesting a relatively late-type classification. Evidence for strong spiral arm structure is not apparent, implying either a face-on orientation obscuring such features or a classification as a lenticular galaxy. The overall color profile suggests a mix of stellar populations, with the yellow and orange hues indicating the presence of older, cooler stars, and the bluer hints hinting at ongoing, but low levels of star formation. There is no strong indication of any major mergers or significant disturbances in the galaxy's morphology. 
