The galaxy presents a smooth, elliptical morphology. The central region exhibits a high surface brightness, suggesting a concentrated stellar population. The galaxy appears nearly circular in projection, with only a slight ellipticity. A color gradient is observed, with the central region displaying a yellowish hue, potentially indicative of an older stellar population or dust obscuration, while the outer regions show a bluer tint, suggestive of younger stars. There is no obvious evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, lacking tidal features or signs of a recent merger event.
