The galaxy presents a largely smooth, elliptical morphology. The light distribution exhibits a high degree of central concentration, with brightness decreasing radially outward from a well-defined nucleus. The galaxy displays a spheroidal shape, appearing nearly round in projection, with only a minor deviation from circular symmetry. There is no indication of prominent spiral arms or a distinct disk structure. The galaxy displays a central bulge, and some fainter, bluer regions of star formation towards the outer regions of the bulge. There is no evidence of ongoing major mergers or significant tidal disturbances. A faint haze surrounds the central region.
