The galaxy presents as a relatively smooth, elliptical morphology with a clear central bulge. The central region exhibits a bright, concentrated luminosity, indicative of a high stellar density. The surrounding disk displays a more diffuse glow. Color gradients suggest a difference in stellar populations; the core appears to be composed of older, redder stars, while the outer regions present a slightly bluer hue, hinting at the presence of younger stellar populations and ongoing, but likely low-level, star formation. There is no prominent evidence of spiral arm structures, bars, or significant dust lanes. The overall structure shows minimal signs of recent major merger events or tidal disturbances. The galaxy appears to be a relatively isolated system exhibiting quiescient activity.
