The galaxy presents a largely smooth, elliptical morphology. It exhibits a generally rounded shape, with a very slight elongation. The color profile appears to be red-shifted, with an orange hue that suggests an older stellar population. There is no obvious spiral structure or prominent dust lanes visible in the image. Indications point to minimal signs of disturbance or merging activity. The galaxy's light is concentrated towards the center, with a gradual decrease in brightness outwards, which is consistent with light dispersion. 
