The galaxy appears as a centrally concentrated object, exhibiting a largely smooth morphology. It has a nearly circular, or perhaps slightly elliptical shape, suggesting it may be classified as an elliptical galaxy. The light profile indicates a relatively uniform brightness distribution, fading gradually towards the edges without any prominent spiral arm structures or distinct features discernible at this resolution. The core appears slightly yellowish, potentially indicating an older stellar population, while the outer regions show hints of bluer tones which may indicate some ongoing star formation. There is no obvious evidence of tidal disturbances or mergers.
