The galaxy presents as a somewhat elliptical morphology, appearing more elongated than perfectly circular, but not exceptionally so. It exhibits a relatively smooth profile, with little discernible structure such as prominent spiral arms or a distinct central bar. The light distribution appears centrally concentrated, suggesting a significant bulge component. Color gradients are subtle, but there is a tendency toward bluer hues in the outer regions and redder tones in the core, hinting at possible variations in stellar populations. There may be some minor disturbances or asymmetries in the galaxy's shape, which would be better investigated with higher resolution imaging. There is no strong evidence of ongoing major mergers or significant tidal interactions with other galaxies in the immediate vicinity. Overall, the galaxy is a fairly quiescent system with a significant spheroidal component.
