The galaxy presents an irregular morphology, appearing somewhat disturbed. It exhibits a central concentration of light that graduates outward, with the highest intensity in the center, hinting at a possible galactic bulge. The overall shape is neither purely elliptical nor a well-defined spiral. There's indication of disrupted or merging features, potentially resulting from a past or ongoing interaction with another galaxy. The color distribution is not uniform, with hints of different stellar populations or varying levels of dust extinction across its structure. There is a dominant orange-yellow hue which transitions into redder areas. The structure presents some smoothness, but is not entirely smooth. There appears to be a faint blue region, as well.
