The galaxy exhibits a generally elliptical morphology, appearing moderately elongated with a cigar-like shape. The light distribution appears relatively smooth, with a bright central bulge that fades outward. Subtle irregularities are observed in its extended halo. Color gradients are apparent, with the central bulge showing a yellowish hue, potentially indicating an older stellar population. The outer regions of the galaxy appear slightly bluer, suggesting the presence of younger stars or ongoing star formation. There may be evidence of minor tidal disturbances or interactions, indicated by the slight asymmetry in the outer regions, although these are subtle. The galaxy's overall structure suggests it is a relatively massive system undergoing a phase of transitioning from active star formation to a more quiescent state.
