The galaxy appears to be a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that emits strongly, surrounded by a more diffuse halo. The light distribution suggests it is generally spheroidal. There is minimal evidence of spiral arms or a prominent disk-like structure. Faint irregularities are visible, suggesting some minor interaction or disturbance, but no obvious signs of a major merger event are apparent. The galaxy displays a color gradient, with a more yellow hue in the center transitioning to slightly bluer tones in the outer regions. This suggests that the stellar populations may vary with radius, with older, redder stars dominating the core and younger, bluer stars contributing more to the light in the galaxy's periphery.
