The galaxy presents as a generally smooth and concentrated elliptical object. Its morphology appears predominantly spheroidal, with minimal evidence of spiral arm structures or a defined disk. The light distribution suggests a high degree of central concentration, with a bright, relatively small core region, diminishing in intensity outwards. The ellipticity is moderate, with an axis ratio that deviates somewhat from a perfect circle, presenting a slightly elongated shape. The color appears to be relatively red, indicating a population of older stars and/or a significant amount of dust obscuration. There are no obvious signs of active galactic nuclei, strong star formation regions, tidal tails, or major mergers with other galaxies, although minor disturbances cannot be ruled out.
