The galaxy presents as a centrally concentrated, relatively smooth structure with an overall elliptical morphology. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population likely dominating the luminosity output. Moving outwards from the core, the color gradient transitions subtly toward a redder periphery. This suggests a potential decrease in younger, bluer stars in the outer regions, or a possible increase in dust obscuration. The galaxy appears largely undisturbed, lacking prominent spiral arms or tidal features, suggesting it is not currently undergoing a major merger event. There are subtle indications of asymmetry in the outer regions but not enough to define its shape.
