The galaxy presents a largely smooth, elliptical morphology, with a dominant central bulge exhibiting a yellowish hue. The light is concentrated toward the center, suggesting a high stellar density in the core. There is a slight elongation, but the overall shape appears relatively round. While some faint, diffuse features extend outwards, there is no clear evidence of a spiral arm structure or prominent disk. The general appearance indicates that it is likely an evolved system with a low rate of ongoing star formation. Faint blue tinges in the outer regions are possibly indicative of some younger star populations, but they are not a dominant feature. The relative smoothness and lack of significant disturbances suggests it has not undergone a major merger recently.
