The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. The light distribution is generally smooth, lacking any prominent spiral arms or bar structures. The galaxy's shape appears to be somewhat elongated, with a minor axis to major axis ratio suggesting an intermediate ellipticity. A clear color gradient exists, with the central region displaying a yellowish-white hue, indicative of an older stellar population, while the outer regions exhibit a bluer tint suggesting the presence of younger stars. There is a very slight indication of minor tidal features, but its integrity appears largely undisturbed. The object lacks any obvious signs of active star formation, such as HII regions or dust lanes.
