The galaxy appears as a luminous, elliptical object with a relatively smooth morphology. There is a bright central bulge region that dominates the light profile. The outer regions appear to fade gradually into the background, suggesting a lack of distinct spiral arms or significant star-forming regions. The overall color seems to be slightly blue-white, suggesting the presence of a population of relatively young, hot stars, though redder hues are also observed, perhaps indicating an older population. The galaxy exhibits an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. There is no obvious evidence of ongoing major mergers or tidal disturbances, although some minor asymmetries might be present in the outskirts.
