The galaxy presents a largely smooth morphology. The light distribution suggests an elliptical or lenticular type, with minimal evidence of spiral arms or prominent disk features. The galaxy appears mostly rounded, with no significant elongation or tidal distortions visible. The central region exhibits a slightly higher concentration of light, implying the presence of a bulge. Overall, the galaxy shows a relatively undisturbed structure, lacking strong signs of recent mergers or major interactions. Color gradients appear subtle, shifting from a yellow core to a blue hue at the galaxy's furthest visible boundary.
