The galaxy presents a largely smooth, elliptical morphology with a prominent central bulge. The light distribution is concentrated towards the center, exhibiting a gradual decrease in intensity outwards. The overall color is predominantly yellowish-orange, suggesting a stellar population dominated by older, redder stars. There appears to be a faint, diffuse halo surrounding the main body of the galaxy. No distinct spiral arms or significant dust lanes are discernible, reinforcing the classification as an elliptical galaxy. There is very little to no evidence of any significant ongoing merger activity or strong tidal disturbances affecting its overall structure. The galaxy appears relatively isolated, with no obvious nearby companions in close proximity.
