The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape appears to be elliptical, showing a high degree of roundness. There is little evidence of spiral arm structures or a distinct disk component. Light intensity is brightest at the center, gradually decreasing towards the outer edges. The color appears to be a relatively uniform blue-white, hinting at a population of intermediate-age to older stars. There are no obvious signs of a major ongoing merger event or significant tidal disturbances, although the potential for a minor disturbance cannot be ruled out. The galaxy likely has a low star formation rate.
