The galaxy appears to be a relatively luminous elliptical galaxy, exhibiting a smooth, spheroidal morphology with a high degree of central concentration. The galaxy appears roughly circular in shape, with a slight deviation from perfect circularity, potentially indicating some degree of interaction or internal dynamics. There is a subtle color gradient visible, with the central regions appearing slightly more yellow/green, suggesting an older stellar population. No distinct spiral arms or prominent dust lanes are visible, which, along with the concentrated central bulge, is characteristic of early-type galaxies. There is a faint blue region on one side of the galaxy indicating some recent star formation. Faint signs of a disturbance/tidal tail can be seen in this same region. The overall color indicates a significant population of older stars, but the presence of bluer regions suggests ongoing or recent star formation at a moderate rate.
