The galaxy exhibits a complex morphology, possibly resulting from an ongoing or recent interaction. Two distinct luminous regions are discernible, appearing as separate galactic entities or nuclei within a single system. The larger, more diffuse structure shows an elongated shape reminiscent of a spiral galaxy seen at an oblique angle, although no distinct spiral arms are visible. This may be due to the effects of tidal forces. The smaller, more compact region is more uniform in color and intensity, appearing elliptical or spheroidal. The color of the galaxy ranges from blue to red, likely indicating a mix of stellar populations, with bluer regions potentially harboring younger, hotter stars and redder regions dominated by older, cooler stars. There appears to be ongoing star formation, albeit not at a highly vigorous rate. The overall shape is noticeably disturbed, and the image may show evidence of minor tidal features, suggestive of a gravitational interaction.
