The galaxy presents a largely smooth morphology, appearing as a single, relatively concentrated mass of stars. The central region exhibits a yellowish-orange hue, suggesting an older stellar population. There's a subtle color gradient outwards, with hints of blue-green in the outer regions. This suggests a possible, albeit faint, presence of younger stars or ongoing star formation in the galaxy's periphery. The galaxy appears to be primarily spheroidal in shape, with no clear evidence of spiral arms or a prominent disk structure. There is no indication of any major disturbances in the galaxy's structure.
