The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The light profile appears relatively uniform, lacking distinct spiral arms or prominent dust lanes. A slight elongation is observed, suggesting a deviation from perfect sphericity.

The galaxy exhibits a color gradient, transitioning from a yellowish-orange hue in the central region to a subtly bluer tinge in the outer regions. This color variation may imply differences in stellar population ages and metallicities across the galaxy, with older, redder stars dominating the core and younger, bluer stars residing in the periphery. The galaxy displays minimal signs of ongoing star formation. There is no indication of major mergers or tidal disturbances in this image. 
