The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a slightly elongated shape, deviating marginally from perfect circularity. The light distribution suggests a relatively uniform stellar population, indicative of an older system dominated by evolved stars. There is little evidence of significant spiral structure or active star formation regions, although there may be very subtle color variations across the galaxy's body. No clear signs of interaction or tidal disturbances are visible in the immediate vicinity, suggesting it is an isolated system.
