The galaxy presents a complex morphology, appearing neither purely elliptical nor a well-defined spiral. Its central region exhibits a concentrated, bright, yellowish-orange hue, possibly indicating an older stellar population or significant dust obscuration. Extending from the core are fainter, bluish-white tendrils or diffuse arms, suggesting regions of ongoing or recent star formation. There are noticeable disturbances in the structure and possibly a merging event, particularly in the slight asymmetry observed in the morphology. The overall appearance indicates that the galaxy is undergoing some type of interaction or internal dynamical process leading to the disruption of a more regular shape. A notable feature is the patchy or clumpy distribution of light within the galaxy, with the galaxy displaying some degree of overall 'featured' structure. This may be indicative of regions of enhanced star formation, dust clouds, or tidal debris from a past interaction.
