The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a high surface brightness, appearing a bright yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the light gradually diminishes. The surrounding area exhibits a more diffuse and reddish tint, indicating a potentially lower star formation rate in these regions. There's little indication of spiral arms or prominent dust lanes. There's no obvious signs of a major ongoing merger, though minor disturbances are not ruled out. The shape is somewhat elongated, appearing more like a flattened spheroid than a perfect circle. Overall, the galaxy appears to be a relatively evolved system with a dominant smooth stellar distribution.
