The galaxy presents as a somewhat amorphous, low surface brightness object. There's a central concentration of light, suggestive of a bulge component. The overall morphology is difficult to classify definitively, but exhibits some disturbed features. The bluer colors may indicate regions of active star formation, while the redder hues might suggest a population of older stars. The light distribution is not entirely smooth. There might be minor tidal disturbances. The galaxy shows signs of potential interaction. There is no well-defined spiral structure, suggesting a disk galaxy that has undergone disruption or an elliptical galaxy with recent star formation. 
