The galaxy presents as a centrally concentrated object, exhibiting a smooth, diffuse morphology. The light distribution suggests an elliptical shape, though it appears somewhat elongated. The core is bright and yellowish, which may indicate an older stellar population. There is a subtle color gradient from the core outwards, transitioning to a slightly redder hue in the outer regions. No distinct spiral arms or significant dust lanes are discernible, supporting its classification as a relatively smooth, possibly early-type, galaxy. There are no obvious signs of ongoing major mergers or tidal disturbances. The galaxy appears relatively isolated in this image.
