The galaxy presents as a somewhat amorphous, moderately bright object with a concentrated central region. Its morphology suggests a smooth component is dominant, although some disturbed features are apparent. There's a lack of strong spiral arm structure and a general roundness, suggesting it may be a late-stage merger, or an elliptical type with peculiar features. It has a bluish hue in its outer regions, suggestive of some ongoing star formation activity, albeit relatively modest. Overall, the galaxy appears to be experiencing an intermediate level of star formation relative to its mass. It is likely a transitioning system experiencing dynamic processes related to interactions or internal evolution.
