The galaxy appears as a singular, centrally concentrated object with a relatively smooth light distribution. It exhibits a moderate degree of ellipticity, tending towards a more rounded shape but not perfectly spherical. The galaxy's core presents a bright, yellowish-white hue, suggesting a significant population of older stars. The intensity of the light gradually decreases from the core outwards, with a faint reddish halo extending into the surrounding space. There is no visual evidence of prominent spiral arms, bar structures, or significant dust lanes. The overall morphology suggests a possible early-type galaxy, potentially an elliptical or lenticular galaxy. No obvious signs of major merger events or tidal disturbances are apparent, although subtle features may be present but are obscured by the image resolution and distance.
