The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits a near-circular morphology. The core region is intensely bright with a yellow-white hue, suggesting a significant population of older stars. There's a slight color gradient outwards from the core. The surrounding regions appear less luminous, gradually fading into the background. The outer regions show a hint of bluer tones, implying the presence of some younger stars or star-forming regions. Overall, it lacks distinct spiral arm structures or irregular features. The light is relatively uniform with no prominent dust lanes or knots of star formation easily discernible in this image. The structure indicates this may be a fairly massive galaxy with a moderate amount of star formation. There are no indications of any major mergers or significant disturbances.
