The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is a noticeable color gradient, transitioning from a bluer hue at the core to redder tones in the outer regions. The galaxy exhibits high degree of symmetry, without any obvious spiral arm structures or bar features visible. There is no strong indication of dust lanes or significant star formation regions within the observed image. The light distribution is centrally concentrated, suggesting a bulge-dominated system. The overall appearance indicates a relatively evolved galaxy.
