The galaxy presents as a single, concentrated luminous body, with a smooth, well-defined elliptical morphology. The object exhibits a pronounced central bulge, characterized by a yellow hue. The overall color gradient suggests a population of older stars. There is no indication of spiral arm structures or significant dust lanes. The high degree of symmetry indicates a relaxed state, with no prominent tidal tails or distortions suggestive of recent major mergers. The galaxy appears relatively isolated, with no obvious signs of interaction with nearby objects. The apparent smooth profile and elliptical shape suggest it is likely an early-type galaxy.
