The galaxy presents a predominantly smooth morphology. The light distribution appears centrally concentrated, with a gradual decline in intensity moving outwards from the core. The central region displays a yellowish hue, potentially indicating an older stellar population. A bluer color surrounds this core, which could be indicative of more recent, though minimal, star formation. The overall shape approximates a circular symmetry, with no visually apparent major distortions or tidal features. It seems to be an isolated system, showing no strong signs of interaction or ongoing merger events, although slight disturbances may be present. The object’s moderate luminosity suggests it is a galaxy of intermediate mass.
