The galaxy presents as a relatively smooth, elliptical-like structure, although not perfectly round. A central bulge is clearly visible, exhibiting a concentrated luminosity. There is a slight extension or halo surrounding the central region, suggesting a more diffuse distribution of stars in the outer regions of the galaxy. The color profile indicates a mix of stellar populations, with the central region exhibiting warmer, yellower hues. There are no immediately obvious spiral arms or major disturbances.
