The galaxy appears as a moderately bright, elliptical object. It exhibits a smooth, largely featureless morphology with a high degree of central concentration. There is a slight elongation along one axis, deviating marginally from a perfectly circular shape; its shape is more in-between rounded and elongated. There is no visible evidence of spiral arms, rings, or a prominent disk structure. The galaxy's light profile shows a gradual decrease in intensity from the core outwards, indicating a centrally concentrated stellar population. The color appears to be yellowish-orange, suggesting a population of older, redder stars with a low rate of on-going star formation. There is no apparent indication of any major mergers or significant tidal disturbances affecting its structure, though the possibility of minor disturbances cannot be ruled out.
