The galaxy appears as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, showing a high degree of roundness. There are no prominent spiral arms or bar structures visible. The galaxy's core exhibits a brighter, more intense luminosity, suggesting a concentrated central bulge. There are hints of color variation with a subtle gradient from a slightly bluer inner region to a redder outer halo, which could signify differences in stellar populations or dust content. There are possible distortions or minor disturbances in the outer regions of the galaxy, indicating potential past interactions or mergers. However, the galaxy primarily appears isolated with no major signs of ongoing merging activity. The overall smooth morphology and roundness suggest a galaxy that is relatively evolved.
