The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The light distribution suggests a primarily spheroidal shape, appearing nearly circular in projection. There is no discernable spiral structure or prominent disk component visible in this image, supporting a classification as an elliptical or S0 galaxy. The galaxy exhibits a noticeable color gradient, transitioning from a yellowish core region to a slightly redder outer halo. This color gradient implies varying stellar populations, with potentially older, redder stars dominating the outer regions and a possible concentration of younger, bluer stars, or dust, towards the center. No strong signs of recent merger activity or significant tidal disturbances are visually apparent; the overall structure appears relaxed and undisturbed. Based on its color and morphology, the galaxy may be a relatively massive and evolved system.
