The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. The light distribution fades gradually from the center outwards. There is little evidence of spiral arms or prominent dust lanes. The overall shape is approximately round, with only minor deviations from circular symmetry. There do not appear to be any major tidal features or signs of ongoing mergers with other galaxies.
