The galaxy presents a somewhat elliptical morphology with a major axis oriented approximately north-south. Its light profile appears relatively smooth, with a centrally concentrated bulge. A subtle disc may be present, indicated by the slight flattening. Color gradients suggest younger stellar populations in the central regions, indicated by the blue hue, with older, redder populations populating the outer regions. Evidence of only minor disturbances suggests it is not undergoing any major merging activity.
