The galaxy appears as a centrally concentrated object, with a smooth and relatively featureless morphology. The light distribution indicates a dominant bulge component, showing a gradual decrease in intensity from the core outwards, with a nearly circular shape. There is no indication of prominent spiral arms or a well-defined disk structure, rather it appears amorphous. The color profile suggests that the core is bluer than the outer regions. There is no evidence of strong tidal features, suggesting the galaxy is not currently undergoing a major merger event. Overall, the galaxy appears to be an elliptical or lenticular galaxy with a smooth distribution of light and a lack of significant morphological features.
