The galaxy presents a morphology that appears generally smooth, though not perfectly spherical. It exhibits an intermediate ellipticity, tending more towards a cigar shape than a perfectly round form. There is a slight suggestion of a disk-like structure, but no distinct spiral arms are evident. The color profile indicates a relatively high luminosity in the blue and green bands relative to the red, implying a significant population of younger, hotter stars and ongoing star formation. The galaxy does not show major signs of merging activity, but minor disturbances cannot be ruled out. The overall mass is quite high. It is an actively star-forming galaxy.
