The galaxy appears to be an elliptical galaxy, exhibiting a high degree of central concentration with a generally smooth morphology. The light distribution suggests a near-spherical shape. There's no indication of prominent spiral arms or a well-defined disk structure. The central region is brighter and more compact, fading gradually towards the outer edges. The galaxy appears to have a minor asymmetry or disturbance visible in the surrounding area, potentially suggestive of a past interaction. The color is generally consistent across the body of the galaxy suggesting a dominant population of older stars.
