This galaxy presents a largely smooth, elliptical morphology. It is characterized by a bright, concentrated central bulge exhibiting a reddish-orange hue, possibly indicative of an older stellar population. The galaxy's light profile fades gradually outwards from the core. There appears to be a subtle, diffuse halo extending beyond the central region, showing a less pronounced color, possibly composed of a mix of stellar populations. The overall shape appears mostly round. There are no obvious signs of a prominent disk structure or ongoing major merger activity. There is a slight hint of disturbance in the outer halo, though most of the light seems to be concentrated near the center.
