The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is minimal evidence of spiral arm structure or significant disk features. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region, potentially indicative of evolved stars. The outer regions appear slightly bluer, possibly hinting at a lower level of ongoing star formation. The galaxy appears generally undisturbed, showing no prominent signs of tidal interactions or recent major mergers, although subtle asymmetries might be present upon closer inspection. The overall shape is moderately elliptical rather than perfectly spherical.
