The galaxy presents an overall elliptical morphology with a dominant, smooth central bulge exhibiting a yellowish hue, indicating a population of older stars. Fainter extensions are observed around the central bulge, suggesting the presence of a diffuse halo component. There is some visual disturbance or extended feature to the upper left of the galaxy, perhaps a tidal tail or an area of star formation. The asymmetry in the outer regions points to a possible interaction or recent merger event. The galaxy appears relatively compact. The color gradient from the center outwards suggests differing stellar populations.
