The galaxy presents an elliptical morphology, appearing moderately smooth in structure. It is characterized by a prominent central bulge that exhibits a yellowish hue, suggesting a population of older, redder stars. Surrounding this central region is a more diffuse halo or disk, showing bluer tones, which potentially indicates the presence of younger stars and regions of ongoing star formation, although the star formation appears to be relatively low. The galaxy appears largely undisturbed, lacking any obvious signs of recent major mergers or significant tidal interactions with other galaxies. The overall shape is slightly elongated, exhibiting an intermediate roundness. There is no indication of a prominent spiral arm structure or a distinct central bar feature within the galaxy.
