The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. It has a slightly elongated shape. The core appears bright and yellow, indicating an older stellar population. The outer regions exhibit a more subtle color gradient, transitioning to redder hues, potentially indicative of an increasing proportion of older, cooler stars in these areas. There's no clear evidence of spiral arms or significant dust lanes from the image alone, reinforcing its elliptical classification. No merging or tidal disturbances are obviously affecting the overall structure.
