The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, potentially indicative of a supermassive black hole or a dense stellar population. A gradual decrease in luminosity is observed moving outward from the core. The overall color appears to be on the redder side of the spectrum. The shape is close to round. There is no evidence of spiral arms or a significant disk component. The image does not immediately reveal any signs of a major ongoing merger, although the possibility of a minor interaction or past merger cannot be entirely ruled out.
