The galaxy presents a generally smooth appearance with a slightly elongated, cigar-shaped morphology. There's a discernible central bulge that appears brighter and more concentrated than the outer regions. The color gradient suggests an older stellar population dominating the bulge, exhibiting a yellowish-orange hue. The outer regions appear fainter and slightly bluer, possibly indicating the presence of a younger stellar population or some residual star formation. No prominent spiral arms or distinct dust lanes are visible. There is no obvious indication of any major ongoing merger activity, but subtle disturbances in the outer halo cannot be ruled out based on this image alone. Overall, this galaxy appears to be a relatively evolved system, possibly an elliptical or lenticular galaxy observed at a distance, with a smooth distribution of light and a prominent bulge.
