This galaxy appears to be a relatively smooth, centrally concentrated object, likely an elliptical galaxy. It exhibits a largely spheroidal shape, though not perfectly round. The light distribution suggests a bulge-dominated morphology, with a bright, dense core that gradually fades into the outer regions. There is no clear evidence of spiral arms or a distinct disk structure, but there may be a hint of a subtle extended halo. The galaxy displays a color gradient, transitioning from a pale yellowish-white in the central bulge to slightly bluer hues in the outskirts, which may indicate the presence of a younger stellar population in the outer regions, although the overall low levels of star formation suggest that it is most likely due to background noise. There is no noticeable signs of any ongoing major merger activity or significant tidal distortions in the immediate vicinity.
