The galaxy appears to be a relatively smooth, elongated structure. It exhibits a cigar-like shape, lacking significant spiral arm definition. There's a subtle color gradient visible, with a slightly bluer tinge towards the outer regions of the galaxy and a yellowish-white concentration towards the central bulge. The overall light distribution suggests an elliptical or lenticular morphology, where the older stellar population dominates. The galaxy shows no strong signs of major mergers or tidal disturbances. However, some subtle irregularities in the outer regions suggest the possibility of minor gravitational interactions or recent accretion events. Overall, it appears to be a fairly evolved galaxy, consistent with a relatively high degree of smoothness.
