The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. Its shape is approximately elliptical, exhibiting a degree of roundness, with a slight deviation from a perfect circle. The light profile suggests a relatively even distribution of luminosity, fading gradually from the bright, yellowish core to the outer regions. There is no strong evidence of spiral arms or a prominent disk structure, but the yellow-white hue suggests that the stellar population is largely composed of older stars. There is little to no discernible evidence of recent or ongoing major merger events.
