The galaxy presents as an elliptical morphology, appearing largely smooth and concentrated. The core exhibits a bright, yellowish hue, potentially indicative of an older stellar population. Moving outwards from the core, the galaxy transitions into a more diffuse, bluish halo, suggesting the presence of a younger, star-forming population within the galactic disk. There are minor disturbances visible within the disk. The galaxy is moderately rounded in shape, showing some degree of ellipticity.
