The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical. The central region exhibits a bright, yellowish-white hue, which gradually fades into a more diffuse and less luminous outer region exhibiting a slightly redder tint. There is no apparent spiral arm structure or dust lane features. The object's symmetric and concentrated light profile suggests a system dominated by an older stellar population. There's no evidence of significant ongoing star formation activity based on the color information in the image. The galaxy appears isolated, lacking any obvious tidal distortions or signs of recent merger activity.
