This galaxy appears to be a relatively smooth, elliptical system. It presents a centrally concentrated luminosity profile, with a gradual decrease in brightness moving outward from the core. There is little evidence of spiral arm structure or significant dust lanes within the galaxy. The color indices suggest the presence of an older stellar population. The galaxy shows no clear signs of ongoing merger activity or major tidal disturbances in the immediate vicinity. The overall morphology suggests a galaxy that has undergone significant internal evolution, leading to a quiescent state with a low star formation rate. The galaxy appears to be slightly more luminous in the redder bands suggesting it is likely comprised of older stellar populations.
