The observed galaxy presents as a moderately luminous, elliptical morphology. The central bulge exhibits a concentration of light, appearing yellowish-white in color, suggesting an older stellar population. Moving outwards from the core, a subtle color gradient is observable. The extremities of the galaxy show hints of bluer hues, potentially indicating regions of more recent star formation, though this is not strongly pronounced. Overall, the galaxy appears relatively smooth in texture, with no prominent spiral arm structures or obvious signs of major disturbances or mergers readily apparent in the image. The object is elongated in shape, exhibiting an approximately 3:1 axial ratio.
