The galaxy exhibits a generally smooth morphology with a centrally concentrated luminosity profile. It presents an elliptical appearance, with a shape that is observed to be somewhat in between round and elongated. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy’s light is dominated by older stellar populations, giving it a yellowish hue. No strong signs of on-going major mergers or tidal disturbances are apparent, but minor disturbances cannot be ruled out. The galaxy appears relatively isolated in the image.
