The galaxy appears as a single, relatively smooth, and concentrated object. It has a generally elliptical morphology with a high degree of roundness. No distinct spiral arms or other pronounced features are discernible. The central region exhibits a high degree of luminosity. The color profile suggests a galaxy dominated by older stellar populations. There is no evidence of any major merger events or significant tidal disturbances, although minor disturbances may be present. The overall impression is that of a fairly mature, quiescent system with a low rate of star formation.
