The galaxy appears as a centrally concentrated object with a smooth overall morphology. It exhibits a radial color gradient, transitioning from a yellowish core to fainter, bluer outer regions. The isophotes appear generally elliptical, exhibiting a moderate degree of roundness. There is some visual indication of minor disturbances or irregularities in the outer structure, but no strong signs of an ongoing major merger or tidal interactions are evident. Star formation appears present, concentrated in the outer regions, at a relatively low rate.
