The galaxy presents as a relatively smooth, elongated elliptical structure. The central region exhibits a high surface brightness, appearing as a concentrated, bright core. This likely indicates a dense stellar population. Moving outwards from the core, the light gradually diminishes in intensity. The outer regions of the galaxy display a yellowish-red hue which may indicate the presence of an older stellar population or dust extinction. No distinct spiral arm structures are visible. There are no obvious signs of major mergers, though a possible minor disturbance in the outer regions cannot be ruled out. The overall morphology suggests a mature, relatively quiescent galaxy.
