The galaxy presents a largely smooth morphology. It appears approximately elliptical in shape, exhibiting a high degree of central concentration with light gradually diminishing outwards. The core region shows a bright, yellowish hue suggestive of an older stellar population. Fainter greenish colors can be seen in the surrounding region, and a subtle blue tinge in the outermost areas, hinting at the presence of some younger, star-forming regions, though they do not dominate. No obvious spiral arm structures or signs of recent major merger events are visible, though slight irregularities might suggest minor disturbances. Overall, the galaxy’s structure indicates a relatively quiescent, evolved system.
