The observed galaxy presents as a spiral type, displaying a discernible disk structure. The spiral arms are apparent but not tightly wound. A central bulge is present, though not prominently dominant, suggesting a classification leaning towards later-type spirals. There are indications of possible interactions or minor disturbances in the galaxy's morphology, but the galaxy does not appear to be a classic major merger. The galaxy shows general blue color indices, suggesting active star formation is likely occurring within its disk.
