The galaxy presents a smooth, elliptical morphology with a high degree of roundness. It is characterized by a centrally concentrated luminosity profile, diminishing gradually toward the outer regions. Color gradients suggest a potentially older stellar population, with the core exhibiting a yellow-orange hue. There is no visually apparent disk structure or spiral arm features. Evidence for ongoing mergers or significant tidal disturbances appears to be absent. The galaxy exhibits a red shift, indicating it is not within our local group and is at a significant distance.
