This galaxy appears to be an elliptical galaxy, exhibiting a largely smooth morphology without discernible spiral arms or prominent dust lanes. The galaxy presents a concentrated central bulge with a yellowish hue, possibly indicative of an older stellar population. The isophotes appear relatively round, suggesting minimal flattening or distortion. There are no obvious signs of recent or ongoing major merger activity, though a minor disturbance cannot be entirely ruled out. The color gradient shifts subtly from a more yellow/orange core to a slightly bluer outer halo, implying a possible difference in stellar population age or metallicity with radius. Overall, the galaxy seems to be a relatively undisturbed, evolved system.
