The galaxy presents a generally smooth, elliptical morphology. Its light profile appears largely featureless, with no obvious spiral arm structures or distinct dust lanes visible at this resolution. The central region is relatively concentrated, indicated by the higher light intensity in the center compared to the outer regions. A yellow hue dominates the galaxy's color, suggesting a stellar population that is somewhat evolved, with relatively low levels of ongoing star formation. There is some variance in color within the galaxy, particularly in the core where a reddish tint is observed. The galaxy exhibits a relatively high degree of circularity in its overall shape. There is no strong evidence of tidal tails, bridges, or other indications of major merger activity, though subtle minor disturbances or interactions cannot be ruled out based on this image alone.
