The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated distribution of light. It exhibits a near-perfect elliptical morphology, showing a high degree of radial symmetry with only minor deviations from a perfect ellipse. There is no evidence of spiral arm structure or a distinct disk component. The color gradient is subtle, transitioning from a bright, almost white core to a slightly bluer outer halo, suggesting a population of older stars in the central region and perhaps a younger, bluer stellar population in the periphery. No signs of ongoing major merging events are visible, and the galaxy shows only a smooth light distribution indicating a relaxed state.
