The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse morphology with a concentrated central bulge. The light distribution suggests an older stellar population, characterized by a yellowish-orange hue. The isophotes are generally elliptical, with a moderate degree of ellipticity, indicating a flattened shape. There is no discernible spiral structure or dust lanes. The galaxy displays a relatively uniform color gradient, with the central regions appearing slightly brighter and yellower than the outer regions, which fade into a more subdued halo. There's no evidence of significant tidal interactions or morphological disturbances in this image. Overall, it presents as a relaxed, passively evolving system.
