The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated bulge that dominates its overall luminosity profile. There may be a very faint disc component, but the bulge is much more noticeable. The galaxy displays a color gradient, appearing slightly bluer toward the outer regions and trending towards yellower hues near the core, indicative of a transition from ongoing star formation in the outer edges to an older stellar population concentrated in the center. There are some very minor signs of tidal disturbance. The overall structure seems relatively undisturbed, but there appears to be some merging event within the structure of the galaxy, although it does not appear to be a major merger. The light is unevenly distributed, showing subtle variations in brightness across its surface.
