The galaxy presents a relatively smooth, elliptical morphology. It appears highly symmetrical with a concentrated central bulge, exhibiting a gradual decline in luminosity from the core outwards. There is little to no evidence of spiral arm structures or significant dust lanes within the visible spectrum. The color profile suggests an older stellar population with a yellowish to reddish hue, indicative of lower star formation rates. Its structure indicates a generally relaxed and dynamically stable system, without substantial signs of recent or ongoing merger activity or significant tidal disturbances.
