The galaxy presents a somewhat diffuse morphology. Its overall color suggests a composite stellar population, with a notable concentration of older, redder stars towards the central bulge. The presence of a faint, blue-ish halo indicates some ongoing, though perhaps limited, star formation, possibly in the outer regions. There's a subtle asymmetry in the distribution of light, which might hint at a past or ongoing minor interaction, though no strong tidal features or merging signatures are immediately apparent. The galaxy appears to be relatively smooth in structure with, at best, a weak disk component.
