The galaxy presents as a largely featureless, elliptical morphology. Its light profile appears smooth and centrally concentrated, with a noticeable lack of spiral arm structures or distinct dust lanes. The overall shape is somewhat elongated, exhibiting an intermediate ellipticity. The color profile suggests an older stellar population, with a reddish-orange hue dominating the visible spectrum. This is indicative of a galaxy where star formation activity has largely ceased, leading to a prevalence of evolved, red giant stars. There is no obvious indication of ongoing major merger events or significant tidal disturbances in the image. Minor disturbances cannot be ruled out, though no clear evidence is visible.
