The galaxy appears as a moderately bright, elliptical object with a smooth, diffuse light distribution. The central region exhibits a yellowish-gold hue, suggesting an older stellar population. The overall shape is elongated, but not drastically so, indicating a moderate ellipticity. There is no discernible spiral structure or distinct dust lanes. Subtle color gradients are present within the galaxy's body, with a slight shift toward redder tones at the core. There is no strong evidence of ongoing star formation based on the color and morphology. The galaxy seems relatively undisturbed, with no obvious signs of tidal interactions or recent merger events.
