The galaxy presents a roughly face-on spiral morphology. The central bulge exhibits a moderate size relative to the galactic disk. Faint spiral arms extend outwards, exhibiting a patchy and somewhat disturbed structure. The arms have distinct knots of bluer light, indicative of ongoing star formation regions. The overall color suggests a mix of stellar populations, with an older, redder population dominating the bulge and a younger, bluer population within the spiral arms. Some minor distortions in the disk are present, possibly suggesting a past or ongoing interaction. It shows no clear bar structure.
