The galaxy appears as a singular, relatively symmetric object with a high degree of central concentration. The color profile indicates a likely evolved stellar population. The light is primarily in the redder part of the spectrum, shifting towards the green, with only a slight hint of blue light in the center, possibly indicating a small area of younger stars in the core. The morphology is generally smooth, without any obvious spiral arms or a defined disk structure. There are no apparent signs of tidal tails, distortions, or interacting companion galaxies that would suggest recent or ongoing merger activity. It appears mostly elliptical in nature, somewhere in the middle of the roundness scale.