The galaxy presents a smooth, centrally concentrated morphology. The light profile appears largely elliptical, exhibiting a slightly elongated, cigar-like shape. The color distribution displays a radial gradient, transitioning from a yellowish-white core to a bluer, fainter outer halo. There is no obvious indication of spiral arm structures or prominent dust lanes. The overall appearance suggests a relatively evolved system, potentially an elliptical or lenticular galaxy, with ongoing or recent star formation. There appears to be no signs of any major or minor disturbances or ongoing mergers affecting the galaxy's structure.
