The galaxy presents a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated with a bright, unresolved core. The overall color suggests a redder spectral energy distribution, indicative of an older stellar population. There are no prominent spiral arms or dust lanes visible, which is consistent with the lack of ongoing, significant star formation. The galaxy's structure appears largely undisturbed, with no obvious signs of tidal interactions or recent merger events. The ellipticity of the galaxy is minimal, giving it an almost circular appearance. There is a slight color gradient, with the core appearing bluer than the outer regions of the galaxy. This may indicate some younger stars in the core or a different metallicity.
