The galaxy appears to be a spiral galaxy, viewed at an oblique angle. There is evidence of a central bulge which occupies a considerable region of the galaxy. The spiral arms are not sharply defined, suggesting a flocculent structure. The blue color indicates ongoing star formation within the arms, and the overall shape is moderately disturbed. The galaxy is a relatively massive system with an estimated size of approximately 3.5 kpc, experiencing a moderate rate of star formation. There is potential evidence of a bar feature across the central region, but this is obscured by the bulge. A hint of a minor merger event cannot be ruled out, as there appears to be an irregular extension.
