The galaxy presents as an elongated, cigar-shaped structure, with a clear central bulge. It exhibits a smooth, diffuse morphology overall. The color profile suggests a mixture of stellar populations. The central bulge is predominantly yellow/orange, indicating an older, redder population. The outer regions show hints of bluer light, which are likely younger stars, and thus possibly some ongoing star formation. There's no distinct spiral arm structure visible, nor strong evidence of dust lanes. The galaxy doesn't appear to be undergoing any major merging events, though a subtle asymmetry suggests potential minor interactions in its past.
