This galaxy exhibits a generally elliptical morphology, appearing largely smooth in structure. There is evidence of a central region that presents a more complex and irregular structure, possibly indicating ongoing or recent star formation. The colors present suggest the presence of both older stellar populations, contributing to the smoother outer regions, and younger, bluer stars concentrated in the central region. There is also a subtle hint of potential interaction or minor disturbance in the galaxy's form, although the overall appearance remains relatively undisturbed. The galaxy's shape is more rounded than elongated. The light distribution is concentrated towards the center, with a gradual decrease in intensity toward the outer edges.
