The galaxy presents as an elongated structure, approximately 3 arcseconds in its longest dimension. A noticeable color gradient exists along the major axis; one end displays a bluer hue, transitioning to a redder tone towards the opposite end. This suggests differing stellar populations or dust extinction along the galaxy's extent. There's evidence of disturbances in the galaxy's morphology, possibly indicating a recent or ongoing interaction with another galaxy, which appears above it. One end of the galaxy appears more condensed and potentially brighter than the rest, which may be the center of the galaxy. Faint wisps and disrupted structures can be observed. No distinct spiral arm features are immediately apparent. Overall, the galaxy seems to be in a state of transition or disruption.
