This galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. The core region exhibits a brighter, yellowish-white hue, indicating a likely concentration of older stellar populations. The outer regions display a somewhat fainter, more diffuse distribution of light, with a hint of bluer tones at the very edges suggesting the presence of some younger stars or ongoing star formation, though this is not very prominent. Overall, the galaxy lacks any obvious spiral arm structures or significant morphological disturbances, and seems undisturbed. 
