The galaxy presents as a single, concentrated object with a relatively smooth morphology. It appears elliptical in shape, exhibiting a high degree of circular symmetry. The galaxy's core region displays a bright, intense luminosity, suggesting a dense concentration of stars. Moving outwards from the core, the light gradually diminishes, forming a diffuse halo with indistinct boundaries. There is a notable lack of discernible features such as spiral arms or prominent dust lanes. The overall color profile indicates a relatively evolved stellar population, with a reddish hue dominating the galactic light, possibly indicating a reduced rate of ongoing star formation. No signs of tidal tails, mergers, or other significant gravitational interactions are apparent within the immediate vicinity.
