The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. It is nearly face-on, but seems to possess a slight elongation, deviating from perfect circularity. The light profile suggests a dominant bulge component, characterized by a bright, diffuse, yellow-white color. The galaxy appears to be relatively isolated, with little evidence of major ongoing mergers or strong tidal disturbances. Faint, bluish extensions are present in the disk, suggestive of some star formation. 
