The galaxy presents as a generally smooth, elliptical form. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density or an active galactic nucleus. Moving outward from the center, the light gradually diminishes, forming a diffuse halo. The shape is elongated, with a cigar-like appearance rather than perfectly circular. There is no immediately apparent indication of spiral arms or other significant morphological features. Possible minor disturbances can not be ruled out but the galaxy appears to not be undergoing any major mergers. Colors are mainly yellow with redder and more diffuse outskirts. Overall, the galaxy's morphology suggests an evolved stellar population and minimal ongoing star formation.
