The galaxy presents as a smooth, elongated structure with a cigar-like shape. The central region exhibits a higher surface brightness, appearing more concentrated and luminous. A subtle color gradient is discernible, transitioning from a predominantly blue-white core to a more reddish periphery. There appears to be minimal evidence of spiral arm structures or significant dust lanes. The overall morphology suggests a relatively quiescent system, perhaps an elliptical or lenticular galaxy with a modest amount of ongoing star formation. A slight asymmetry in the outer regions might indicate a minor interaction or disturbance, but the dominant impression is one of established equilibrium.
