The galaxy presents a generally smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, appearing yellowish in color. This likely indicates a population of older stars. The galaxy shows a relatively symmetric shape. There are no distinct spiral arms or a prominent disk structure visible. The color appears to become slightly redder moving outwards from the core, which could indicate a radial change in stellar populations or dust content. There are no obvious signs of significant tidal disturbances or major mergers. Subtle irregularities near the outer edges suggest the possibility of minor interactions or internal structures, but are not well-defined in the image resolution.
