The galaxy presents a complex morphology, possibly indicative of an ongoing or recent merger event. There is a primary, somewhat spheroidal component exhibiting a diffuse light profile, with a distinct bluish hue, suggesting the presence of younger stellar populations and ongoing star formation. A fainter, more elongated structure appears connected to the main body of the galaxy. This secondary structure displays a gradient in color, transitioning from blue at the apparent connection point to a yellowish-white at its distal end. This color variation could be due to differential star formation or dust extinction along the structure. The overall shape is irregular, deviating significantly from a simple elliptical or spiral form. Patches of enhanced luminosity are observed within the primary component, potentially indicating regions of active star formation.
