The galaxy presents as a disk galaxy with a moderate inclination relative to our line of sight. The central bulge appears yellowish and moderately prominent, gradually fading into the surrounding disk. The disk exhibits a faint spiral structure, with two main arms discernible. These arms display a medium winding, extending from the inner regions outwards. Evidence of star formation is suggested by subtle blue hues within the spiral arms. The galaxy does not exhibit any major signs of interactions or disturbances; it shows no obvious tidal tails or distortions that might indicate an ongoing merger, although there is potentially minor asymmetry suggestive of possible past interaction. Overall, the morphology suggests a relatively quiescent galaxy with ongoing star formation within its spiral arms.
