The galaxy presents as a relatively smooth, centrally concentrated system. It exhibits a primarily elliptical morphology, appearing largely spheroidal with a high degree of roundness. A bright, yellowish core dominates the galaxy's central region, indicative of a high stellar density. The galaxy shows a gradual decrease in luminosity from the core outwards, transitioning into a fainter, more diffuse halo. There is some slight evidence of a faint, extended disk-like structure, but this is not clearly defined. No obvious signs of strong tidal interactions or major merger events are apparent. Subtle irregularities in the outer regions may suggest minor disturbances or past interactions, but the galaxy's overall structure appears well-relaxed. The galaxy has an integrated color profile that trends redder at its core.