The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light distribution. The core exhibits a yellowish hue, suggesting an older stellar population. The radial light profile appears to decrease relatively smoothly from the center outwards. There is minimal evidence of spiral arm structures or prominent dust lanes within the visible light spectrum. The overall round shape and lack of significant distortions suggest that the galaxy is relatively undisturbed and has not undergone major mergers recently. Faint, diffuse light extending beyond the central region indicates the presence of a stellar halo. Overall, the galaxy appears to be a mature elliptical galaxy with little current star formation activity.
