The galaxy presents a largely smooth, elliptical morphology. The central region displays a concentrated luminosity with a yellowish hue, suggesting a population of older stars. Progressing outward from the core, there's a subtle fading of intensity. The overall color gradient indicates a transition from a more aged stellar population at the core to a slightly younger population in the outer regions. There are no prominent spiral arms or dust lanes discernible. Subtle irregularities along the edge suggest possible minor gravitational interactions. Overall, the galaxy appears to be a relatively relaxed system, with a fairly regular structure.
