The galaxy presents as a lenticular or early-type spiral, exhibiting a predominantly smooth morphology. There is a slight elongation, though the object tends towards roundness. The galaxy's color profile suggests an older stellar population with a redder overall hue, yet hints of blue indicate some ongoing, albeit limited, star formation. The light is generally concentrated towards the center, with a gradual falloff in brightness as one moves outward, which indicates a large mass. There may be very small features or disturbances in the galaxy's structure, indicative of minor interactions or past mergers, but these do not significantly disrupt the dominant smooth characteristic.
