The galaxy appears as a single, centrally concentrated object with a smooth morphology. The light distribution suggests an elliptical shape, as there is no clear spiral arm structure visible. There is a noticeable color gradient, with the central region exhibiting a yellowish-white hue, suggesting an older stellar population. The galaxy does not appear to be undergoing any major merger events or significant disturbances in its structure. The light profile fades smoothly from the center outwards with no clear features.
