The galaxy presents as a relatively smooth and luminous object, with an elliptical or lenticular morphology. The central bulge appears dominant, characterized by a concentrated, yellowish-orange hue, indicative of an older stellar population. There is a subtle falloff in luminosity and color as we move away from the center. It presents as a fairly symmetric shape, though it is slightly elongated, not perfectly spherical. There are no apparent spiral arms or significant dust lanes visible in this image. There is no evidence of a major ongoing merger. There is no presence of any tidal tails, bridges, or other features associated with gravitational interactions. 
