The galaxy presents a generally smooth, elliptical morphology. It is relatively round in appearance, showing minimal elongation. The central region exhibits a concentrated, bright core that gradually diffuses outwards into a less intense halo. The color profile is generally consistent, with a slight red-yellowish hue, suggesting a population of older stars with minimal ongoing star formation. There is no discernible spiral structure, bar, or other distinct features such as tidal tails or obvious signs of interaction with another galaxy. The galaxy appears to be relatively isolated and undisturbed.