The galaxy presents as a generally smooth, centrally concentrated object. Its morphology appears largely spheroidal, exhibiting a high degree of circularity. The galaxy displays a pronounced central bulge that dominates its overall luminosity. The color profile suggests a relatively evolved stellar population within the bulge, trending towards redder hues. Surrounding the bulge, a fainter, more diffuse halo is visible, showing bluer colors which may indicate ongoing, albeit moderate, star formation activity in the outer regions. There's no clear evidence of spiral arm structure or significant dust lanes. The general appearance indicates a relatively undisturbed system, showing no strong signs of recent major mergers or tidal interactions. Small signs of disturbance might be present but it is difficult to tell based on the resolution of the image.
