The galaxy presents an elongated, cigar-like morphology, suggesting an edge-on or highly inclined disk structure. Its light profile appears relatively smooth, with a concentrated central bulge or core. There is a subtle color gradient, with the central regions appearing more yellowish-orange, possibly indicating an older stellar population or dust obscuration. The outer regions exhibit a slightly bluer hue, hinting at the presence of younger, hotter stars. There is no obvious indication of active star formation regions or prominent spiral arm structures in this image. The overall appearance suggests a galaxy with a significant spheroidal component and a relatively quiescent star formation history. There is no evidence of a major ongoing merger. There may be a hint of minor tidal disruption visible.
