The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile that gradually fades toward the edges. The central region is dominated by a yellowish-orange hue, suggestive of an older stellar population. The isophotes appear largely regular, with only a slight elongation. A faint disk-like structure surrounds the central bulge, showing signs of ongoing or recent star formation indicated by bluer colors within it. There seems to be a slight disturbance in the galaxy's symmetry which could be from a tidal interaction or a minor merger event.
