This galaxy exhibits a prominent disk structure with a relatively small bulge. Distinct spiral arms are visible, indicative of ongoing star formation. There appears to be a bar-like structure traversing the central region, displaying a moderate strength. The galaxy’s morphology appears largely undisturbed, without significant signs of major mergers. There may be some subtle indications of minor gravitational interaction or tidal disturbances in its structure, though the overall appearance suggests a relatively isolated and stable system. The estimated apparent size suggests that the galaxy is moderately compact. The color distribution suggests varying stellar populations, with bluer regions associated with younger stars and redder regions linked to older stellar populations. The galaxy displays a generally smooth appearance with some regions of enhanced star formation activity.
