The galaxy presents an elliptical morphology with a smooth, concentrated central bulge. The light distribution appears relatively uniform across the structure, lacking prominent spiral arms or distinct features. The color gradient suggests an older stellar population, exhibiting a reddish hue with the possibility of ongoing, but low, star formation. The absence of clear dust lanes or prominent blue regions indicates a dearth of active star-forming regions. The overall structure seems undisturbed, showing no obvious signs of recent mergers or major tidal interactions. The galaxy appears to be a massive system and appears to be inclined slightly on the plane of the sky, giving it a somewhat elongated appearance.
