The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its light profile suggests a significant bulge component, with a gradual decline in luminosity outward from the center. The color is predominantly yellow, indicative of an older stellar population. There is no clear evidence of spiral arms, dust lanes, or ongoing star formation regions within the observed wavelengths. The overall shape suggests a relaxed system, with minimal signs of recent mergers or tidal disturbances.
