The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white luminosity, suggesting a high density of older stellar populations. The overall shape is somewhat elongated, exhibiting a moderate ellipticity. The surrounding halo displays a faint, diffuse bluish hue that gradually fades into the background. There are no clear indications of spiral arms or a disk structure. Slight asymmetry is visible with a faint, small appendage or potential tidal feature, which is indicative of a possible past interaction or minor disturbance.
