The galaxy exhibits an elliptical morphology, appearing relatively smooth with no discernible spiral arms or prominent disk structure. The light is concentrated towards the center. The overall color is relatively uniform, with a slight blueish hue in the central region and a gradient towards slightly redder colors in the outer regions, suggesting the presence of older stellar populations. The galaxy has a high Sersic index, suggesting a higher concentration of light and more gradual transition in intensity from the center outwards than would be expected in a disk galaxy. The observed axis ratio indicates a moderately elongated shape. There are no signs of ongoing major mergers or significant tidal disturbances.
