This galaxy appears to be an elliptical or lenticular type, exhibiting a centrally concentrated bulge and a smoother, less defined structure. The galaxy displays a yellowish-orange hue at its core, potentially indicating an older stellar population. Fainter bluish regions surround the central bulge, suggesting the presence of younger, hotter stars or regions of more recent star formation in the outer disk. There are apparent disturbances in the outer regions of the galaxy, potentially indicating tidal interactions or a minor merger event. The disk appears to be more extended along one axis, suggesting a slightly elongated shape and a moderate amount of rotational support.
