The galaxy presents a generally elliptical morphology, appearing relatively smooth and centrally concentrated. There is a noticeable color gradient, transitioning from a slightly yellower central region to a bluer outer halo. The galaxy exhibits a high degree of symmetry. No distinct spiral arm structures or prominent dust lanes are evident. The overall structure suggests a relaxed, evolved system, potentially an elliptical galaxy with ongoing or recently quenched star formation activity. There are no signs of any major mergers or tidal disturbances visible in the current imaging resolution. The galaxy appears isolated within its local field, showing no immediate interaction with neighboring galaxies.
