The galaxy appears as a centrally concentrated object, with a smooth, relatively featureless morphology. The light distribution suggests an elliptical or lenticular galaxy type. There is no obvious spiral structure or distinct dust lanes visible in the image. The galaxy exhibits a radial color gradient, appearing more yellow-orange towards the core, suggesting an older stellar population in this region. The outer regions of the galaxy are fainter and appear slightly bluer, indicating the presence of younger stars or a lower metallicity stellar population. There is no evidence of any significant ongoing merger activity or tidal disturbances from the surrounding environment. The galaxy appears to be isolated and well-defined. The galaxy exhibits an apparent angular size of approximately 3 arcseconds.
