The galaxy presents as a centrally concentrated object with a smooth morphology, displaying a noticeable lack of distinct spiral arm structures or irregular features. The central region exhibits a high degree of luminosity, appearing yellowish-white, suggesting a population of older stars. The outer regions of the galaxy fade into a less luminous halo, indicating a gradual decrease in stellar density with increasing radial distance. The shape appears to be generally elliptical and moderately rounded. There is no obvious indication of tidal tails or significant distortions that would suggest recent major merger events. However, there are possible signs of minor disturbances or irregularities in the outer halo, and possible low level star formation activity based on the color.
