The galaxy presents as a somewhat diffuse object, exhibiting characteristics that place it between a purely elliptical and a spiral form. It appears mostly smooth in overall structure, yet subtle features are present, hinting at a possible disk component. The central bulge is moderately bright and slightly elongated. The outer regions of the galaxy appear fainter and bluer, suggesting the presence of a younger stellar population and ongoing star formation. There might be very minor disturbances, as the object is somewhat irregular in shape, but does not seem to be undergoing a major merging event. The galaxy's overall color index suggests a mixture of stellar populations, with both older, redder stars in the bulge and younger, bluer stars in the outer regions.
